{ "count": 303, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22BEST%22", "previous": null, "results": [ { "id": 31388, "url": "https://svs.gsfc.nasa.gov/31388/", "result_type": "Hyperwall Visual", "release_date": "2026-04-08T12:00:00-04:00", "title": "AVATAR: A Virtual Astronaut Tissue Analog Response", "description": "The AVATAR (A Virtual Astronaut Tissue Analog Response) investigation on Artemis II uses organ-on-a-chip devices, or organ chips, to study the effects of increased radiation and microgravity on human health.", "hits": 1385 }, { "id": 31386, "url": "https://svs.gsfc.nasa.gov/31386/", "result_type": "Hyperwall Visual", "release_date": "2026-04-02T12:00:00-04:00", "title": "Space Station Research Informs New FDA-Approved Cancer Therapy", "description": "European Space Agency (ESA) astronaut Thomas Pesquet works with Protein Crystallization Facility hardware, used to study protein crystal growth research on the space station.", "hits": 1103 }, { "id": 14989, "url": "https://svs.gsfc.nasa.gov/14989/", "result_type": "Produced Video", "release_date": "2026-03-18T09:55:00-04:00", "title": "Hubble Accidentally Catches Comet Breaking Up", "description": "In a happy twist of fate, NASA’s Hubble Space Telescope just witnessed a comet in the act of breaking apart. The chance of that happening while Hubble watched is extraordinarily miniscule. Comet K1, whose full name is Comet C/2025 K1 (ATLAS)—not to be confused with interstellar comet 3I/ATLAS—was not the original target of the Hubble study.Before it fragmented, K1 was likely a bit larger than an average comet, probably around 5 miles across. The team estimates the comet began to disintegrate eight days before Hubble viewed it. Hubble took three 20-second images, one on each day from November 8 through November 10, 2025. As it watched the comet, one of K1’s smaller pieces also broke up. Because Hubble’s sharp vision can distinguish extremely fine details, the team could trace the history of the fragments back to when they were one piece. That allowed them to reconstruct the timeline. But in doing so, they uncovered a mystery: Why was there a delay between when the comet broke up and when bright outbursts were seen from the ground? When the comet fragmented and exposed fresh ice, why didn’t it brighten almost instantaneously?Sometimes the best science happens by accident!For more information, visit science.nasa.gov/mission/hubbleCredit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerOriginal Story Written by: Ann Jenkins / Christine Pulliam of the Space Telescope Science InstituteVideo Credits:Milky Way with comets timelapse. Credit: POND5Comet Shoemaker Levy colliding with Jupiter from ESA's movie \"15 Years of Discovery\". Credit: ESA/Hubble (M. Kornmesser & L. L. Christensen)Comet K1 Image. Credit: NASA, ESA, D. Bodewits (Auburn). Image processing: J. DePasquale (STScI).Diagram of K1’s path through the Solar System. Credit: NASA, ESA, R. Crawford (STScI)Music Credit:“Le nozze di Figaro” by Wolfgang Amadeus Mozart via Chappell Recorded Music Library Ltd [PRS] and Universal Production Music || ", "hits": 310 }, { "id": 31347, "url": "https://svs.gsfc.nasa.gov/31347/", "result_type": "Hyperwall Visual", "release_date": "2026-03-03T18:59:59-05:00", "title": "Astronaut Don Pettit’s Photos from Space", "description": "hyperwall hwshows for photos from https://www.nasa.gov/gallery/astronaut-don-pettits-photos-from-space/", "hits": 1140 }, { "id": 40548, "url": "https://svs.gsfc.nasa.gov/gallery/solarand-heliospheric-observatory-soho/", "result_type": "Gallery", "release_date": "2026-03-03T00:00:00-05:00", "title": "SOHO – Solar and Heliospheric Observatory", "description": "Launched in December 1995, the Solar and Heliospheric Observatory (SOHO) is a joint mission between NASA and ESA (European Space Agency) designed to study the Sun inside out. Though its mission was originally scheduled to last until 1998, SOHO continues to collect observations about the Sun’s interior, the solar atmosphere, and the constant stream of solar particles known as the solar wind, adding to scientists' understanding of our closest star and making many new discoveries, including finding more than 5,000 comets.\n\nLearn more: https://science.nasa.gov/mission/soho/", "hits": 496 }, { "id": 40544, "url": "https://svs.gsfc.nasa.gov/gallery/hinode/", "result_type": "Gallery", "release_date": "2026-02-27T00:00:00-05:00", "title": "Hinode (Solar-B)", "description": "Hinode (Solar-B) is an international mission, led by the Japan Aerospace Exploration Agency (JAXA), to study the Sun. Hinode explores the magnetic fields of the Sun, from tracking their strength and direction on the solar surface, or photosphere, to decoding their role in heating and powering eruptions in the Sun’s outer atmosphere, or corona, to driving the constant outflow from the Sun, the solar wind. \n\nThe mission launched on Sept. 23, 2006, from Uchinoura Space Center in Japan aboard a JAXA M-V rocket.\n\nLearn more: https://science.nasa.gov/mission/hinode/", "hits": 41 }, { "id": 5591, "url": "https://svs.gsfc.nasa.gov/5591/", "result_type": "Visualization", "release_date": "2025-12-29T14:00:00-05:00", "title": "ICESat-2 Land Ice Height Change (2020-2025)", "description": "NASA’s ICESat-2 satellite measures the elevation of Earth’s surfaces – and two data products from the mission map the height of Antarctic and Greenland ice sheets, as well as how those ice sheets change over time. The ICESat-2 ATL14 data product provides a reference ice sheet surface, while ATL15 provides elevation changes to that surface through time.", "hits": 303 }, { "id": 5524, "url": "https://svs.gsfc.nasa.gov/5524/", "result_type": "Interactive", "release_date": "2025-05-22T08:00:59-04:00", "title": "\"Snap It!\" Solar Eclipse Photography Game", "description": "The Traveler needs your help! They have come to Earth to study an event we call a total solar eclipse. Can you help the Traveler snap photos of an eclipse?", "hits": 63 }, { "id": 14835, "url": "https://svs.gsfc.nasa.gov/14835/", "result_type": "Produced Video", "release_date": "2025-05-09T15:00:00-04:00", "title": "What Happened During the Biggest Geomagnetic Storm in Over 20 Years", "description": "On May 10, 2024, the first G5 or “severe” geomagnetic storm in over two decades hit Earth. The event did not cause any catastrophic damages, but it did produce surprising effects on Earth. The storm, which has been called the best-documented geomagnetic storm in history, spread auroras to unusually low latitudes and produced effects spanning from the ground to near-Earth space. Data captured during this historic event will be analyzed for years to come, revealing new lessons about the nature of geomagnetic storms and how best to weather them.Learn more:• What NASA Is Learning from the Biggest Geomagnetic Storm in 20 Years• How NASA Tracked the Most Intense Solar Storm in Decades || ", "hits": 537 }, { "id": 14824, "url": "https://svs.gsfc.nasa.gov/14824/", "result_type": "Produced Video", "release_date": "2025-04-24T09:55:00-04:00", "title": "Hubble’s Highlights from its 35th Year in Orbit", "description": "The Hubble Space Telescope celebrated its 35th year in orbit by premiering four stunning new Hubble images.From the planet Mars, to spectacular star forming regions, to a magnificent neighboring galaxy, these new images are the best birthday present anyone could ask for!Even after all these years, Hubble continues to uncover the mysteries of the universe. These are a few science achievements from Hubble’s latest year in orbit.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerVideo Credit:Images/Visualizations: NASA, ESA, STScIFU Orionis Disk Illustration from NASA Jet Propulsion Laboratory via Caltech/T. Pyle (IPAC)Music Credit:“Quartet for Strings in C Major Emperor\" by Franz Joseph Haydn [DP] and Jim Long [ASCAP], via Just Classics [ASCAP] and Universal Production Music. || ", "hits": 88 }, { "id": 14791, "url": "https://svs.gsfc.nasa.gov/14791/", "result_type": "Produced Video", "release_date": "2025-03-10T06:00:00-04:00", "title": "NASA Interview Opportunity: Watch A Red Moon Dance Across The Sky THIS Friday", "description": "Scroll down page for associated cut b-roll for the live shots and pre-recorded soundbites || Lunar_eclipse.png (1600x640) [480.7 KB] || Lunar_eclipse_print.jpg (1024x409) [85.1 KB] || Lunar_eclipse_searchweb.png (320x180) [65.5 KB] || Lunar_eclipse_thm.png [6.7 KB] || ", "hits": 172 }, { "id": 5515, "url": "https://svs.gsfc.nasa.gov/5515/", "result_type": "Visualization", "release_date": "2025-03-07T00:00:00-05:00", "title": "2024 Atlantic Hurricane Season (Vertical Mode)", "description": "Example composite of how this data visualization might be used on a vertical display. || hurr2024_vert_comp.1000_print.jpg (1024x1820) [651.3 KB] || hurr2024_vert_comp.1000_searchweb.png (320x180) [111.5 KB] || hurr2024_vert_comp.mp4 (1080x1920) [239.3 MB] || composite [0 Item(s)] || hurr2024_vert_comp.1000_thm.png [7.6 KB] ||", "hits": 30 }, { "id": 5468, "url": "https://svs.gsfc.nasa.gov/5468/", "result_type": "Visualization", "release_date": "2025-02-11T18:59:59-05:00", "title": "2024 Atlantic Hurricane Season", "description": "SST, IMERG, CPC, and Hurricane tracks for the entire 2024 Hurricane Season. Also providing separate visualizations of just SST with tracks, IMERG with tracks, and CPC with tracks.", "hits": 178 }, { "id": 14753, "url": "https://svs.gsfc.nasa.gov/14753/", "result_type": "Produced Video", "release_date": "2025-01-13T10:14:00-05:00", "title": "Astronomers Track Jet Launch, Fluctuating X-Rays from Brink of Active Black Hole", "description": "Active galaxy 1ES 1927+654, circled, has exhibited extraordinary changes since 2018, when a major outburst occurred in visible, ultraviolet, and X-ray light. The galaxy harbors a central black hole weighing about 1.4 million solar masses and is located 270 million light-years away.Credit: Pan-STARRSUnannotated versions available.Image description: On a mottled black background, soft circles ranging in color from blue-white to orange represent stars in our own galaxy. At center, to the right of a chain of three bluish stars, lies a softer white circle set within a grayish ellipse whose longest dimension is oriented vertically. This is 1ES 1927+654, circled in green in this image. || 1ES1927_PanSTARRS_1080_circ.jpg (1920x1080) [597.2 KB] || 1ES1927_PanSTARRS_1080.jpg (1920x1080) [591.5 KB] || 1ES1927_PanSTARRS_2160.jpg (3840x2160) [1.7 MB] || 1ES1927_PanSTARRS_1080_circ_searchweb.png (320x180) [87.7 KB] || 1ES1927_PanSTARRS_1080_circ_thm.png [8.9 KB] || ", "hits": 180 }, { "id": 14698, "url": "https://svs.gsfc.nasa.gov/14698/", "result_type": "Produced Video", "release_date": "2024-10-22T11:00:00-04:00", "title": "NASA Reveals LISA Engineering Development Unit Telescope", "description": "NASA has revealed the first look at a full-scale prototype for six telescopes that will enable, in the next decade, the space-based detection of gravitational waves — ripples in space-time caused by merging black holes and other cosmic sources.The LISA (Laser Interferometer Space Antenna) mission is led by ESA (European Space Agency) in partnership with NASA to detect gravitational waves by using lasers to measure precise distances — down to picometers, or trillionths of a meter — between a trio of spacecraft distributed in a vast configuration larger than the Sun. Each side of the triangular array will measure nearly 1.6 million miles, or 2.5 million kilometers.Twin telescopes aboard each spacecraft will both transmit and receive infrared laser beams to track their companions, and NASA is supplying all six of them to the LISA mission. The prototype, called the Engineering Development Unit Telescope, will provide guidance as engineers and scientists work toward building the flight hardware.In May, the prototype, which was manufactured and assembled by L3Harris Technologies in Rochester, New York, arrived at NASA's Goddard Space Flight Center in Greenbelt, Maryland. The primary mirror is coated in gold to better reflect the infrared lasers and to reduce heat loss from a surface exposed to cold space since the telescope will operate best when close to room temperature. The prototype is made entirely from an amber-colored glass-ceramic called Zerodur, manufactured by Schott in Mainz, Germany. The material is widely used for telescope mirrors and other applications requiring high precision because its shape changes very little over a wide range of temperatures. || ", "hits": 118 }, { "id": 5377, "url": "https://svs.gsfc.nasa.gov/5377/", "result_type": "Visualization", "release_date": "2024-09-23T00:00:00-04:00", "title": "Accumulated Hurricane Tracks 1900 to 2023", "description": "Atlantic hurricanetracks that pass through the Caribbean Sea. A ten year window of tracks are shown with tracks closer to the latest year in the window more opaque. The window goes from 1890-1900 until 2013-2023.These equireceangular projections can be wrapped to a sphere. || hurricane_tracks_by_year_equirectangular_caribbean_8k.03100_print.jpg (1024x512) [131.5 KB] || hurricane_tracks_by_year_equirectangular_caribbean_8k.03100_searchweb.png (320x180) [76.5 KB] || hurricane_tracks_by_year_equirectangular_caribbean_8k.03100_web.png (320x160) [69.2 KB] || caribbean [0 Item(s)] || hurricane_tracks_by_year_equirectangular_caribbean_2048p30.mp4 (4096x2048) [66.6 MB] || hurricane_tracks_by_year_equirectangular_caribbean_4096p30_h265.mp4 (8192x4096) [80.4 MB] || hurricane_tracks_by_year_equirectangular_caribbean_4096p30_h265.mp4.hwshow [229 bytes] || ", "hits": 705 }, { "id": 14686, "url": "https://svs.gsfc.nasa.gov/14686/", "result_type": "B-Roll", "release_date": "2024-09-18T11:00:00-04:00", "title": "Eclipse Ballooning Project Featuring the University of Maryland", "description": "The NASA-sponsored Nationwide Eclipse Ballooning Project (NEBP) immerses teams of STEM learners from a wide range of higher education institutions in an innovative NASA-mission-like adventure in data acquisition and analysis through scientific ballooning during the Oct. 14, 2023, annular and April 8, 2024, total solar eclipses.NEBP includes development and implementation of two learner-centered activity tracks – engineering and atmospheric science. At sites along the eclipse path, student teams in the engineering track use innovative larger balloon systems to live stream video to the NASA eclipse website, observe in situ perturbations in atmospheric phenomena, and conduct individually designed experiments. Atmospheric science track teams make frequent observations by launching hourly radiosondes on helium-filled weather balloons. Student participants work with atmospheric science experts throughout the project and will publish results in peer-reviewed journals.The project fully supports 53 teams divided into nine pods to facilitate effective education. NEBP provides a learning environment that uses evidence and equity-based practices to make certain the 750+ participants are (and feel) supported, engaged, and valued. In addition, NEBP provides infrastructure tools and best practices to help participating institutions build collaborations that could continue far beyond the scope of this project.Learn more: https://science.nasa.gov/sciact-team/nationwide-eclipse-ballooning-project/ || ", "hits": 33 }, { "id": 5305, "url": "https://svs.gsfc.nasa.gov/5305/", "result_type": "Visualization", "release_date": "2024-07-02T08:00:00-04:00", "title": "2023 Atlantic Hurricane Season", "description": "The 2023 Atlantic Hurricane Season from June 1st through October 31st. The colors over the ocean are Sea Surface Temperatures where reds are high temperatures and blues are low. The colors underneath the clouds are precipitation measurements, where red is high and greens are low. Each hurricane name tracks with it's corresponding storm and leaves behind category designations (TD=Tropical Depression; TS=Tropical Storm; and 1 through 5 are hurricane strengths) as each storm increases and decreases in strength. || hurr2023_v34_ALL_2024-06-26_1103.00001_print.jpg (1024x576) [234.5 KB] || hurr2023_v34_ALL_2024-06-26_1103.00001_searchweb.png (320x180) [101.0 KB] || hurr2023_v34_ALL_2024-06-26_1103.00001_thm.png (80x40) [6.8 KB] || hurr2023_v34_ALL_2024-06-26_1103_1080p30.webm (1920x1080) [44.7 MB] || All_Data_in_HD [0 Item(s)] || hurr2023_v34_ALL_2024-06-26_1103_1080p30.mp4 (1920x1080) [739.1 MB] || ALL_Data_in_UHD [0 Item(s)] || hurr2023_v34_ALL_4k.mp4 (3840x2160) [2.3 GB] || ", "hits": 53 }, { "id": 31288, "url": "https://svs.gsfc.nasa.gov/31288/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb, Chandra, Hubble, and Spitzer Together Explore Cassiopeia A", "description": "For the first time astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study the well-known supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure in the debris from the destroyed star called the “Green Monster”, first discovered in Webb data in April 2023. The research has also uncovered new details about the explosion that created Cas A about 340 years ago, from Earth’s perspective.A new composite image contains X-rays from Chandra (blue), infrared data from Webb (red, green, blue), and optical data from Hubble (red and white). The outer parts of the image also include infrared data from NASA’s Spitzer Space Telescope (red, green and blue). The outline of the Green Monster can be seen by mousing over the image in the original feature, located here: chandra.cfa.harvard.edu/photo/2024/casa/.The Chandra data reveals hot gas, mostly from supernova debris from the destroyed star, including elements like silicon and iron. In the outer parts of Cas A the expanding blast wave is striking surrounding gas that was ejected by the star before the explosion. The X-rays are produced by energetic electrons spiraling around magnetic field lines in the blast wave. These electrons light up as thin arcs in the outer regions of Cas A, and in parts of the interior. Webb highlights infrared emission from dust that is warmed up because it is embedded in the hot gas seen by Chandra, and from much cooler supernova debris. The Hubble data shows stars in the field.Detailed analysis by the researchers found that filaments in the outer part of Cas A, from the blast wave, closely matched the X-ray properties of the Green Monster, including less iron and silicon than in the supernova debris. This interpretation is apparent from the color Chandra image, which shows that the colors inside the Green Monster’s outline best match with the colors of the blast wave rather than the debris with iron and silicon. The authors conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it, supporting earlier suggestions from the Webb data alone.The debris from the explosion is seen by Chandra because it is heated to tens of millions of degrees by shock waves, akin to sonic booms from a supersonic plane. Webb can see some material that has not been affected by shock waves, what can be called “pristine” debris.Read more here: chandra.cfa.harvard.edu/photo/2024/casa/. || 53453268481_e80cfca2d4_o.jpg (4200x3386) [7.1 MB] || 53453268481_e80cfca2d4_o_searchweb.png (320x180) [121.1 KB] || 53453268481_e80cfca2d4_o_thm.png (80x40) [15.9 KB] || webb-chandra-hubble-and-spitzer-all-explore-cassiopeia-a-composite-all-4.hwshow || ", "hits": 316 }, { "id": 31293, "url": "https://svs.gsfc.nasa.gov/31293/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb, Hubble Telescopes Affirm Universe's Expansion Rate", "description": "This image of NGC 5468, a galaxy located about 130 million light-years from Earth, combines data from the Hubble and James Webb space telescopes. This is the farthest galaxy in which Hubble has identified Cepheid variable stars. These are important milepost markers for measuring the expansion rate of the universe. The distance calculated from Cepheids has been cross-correlated with a type Ia supernova in the galaxy. Type Ia supernovae are so bright they are used to measure cosmic distances far beyond the range of the Cepheids, extending measurements of the universe's expansion rate deeper into space.CreditsNASA, ESA, CSA, STScI, Adam G. Riess (JHU, STScI) || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw_print.jpg (1024x576) [160.4 KB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb.png (3214x3233) [16.1 MB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw.png (3840x2160) [7.7 MB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw_searchweb.png (320x180) [58.9 KB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw_thm.png (80x40) [8.5 KB] || webb-hubble-telescopes-affirm-universes-expansion-rate.hwshow [366 bytes] || ", "hits": 296 }, { "id": 31287, "url": "https://svs.gsfc.nasa.gov/31287/", "result_type": "Hyperwall Visual", "release_date": "2024-06-12T00:00:00-04:00", "title": "Webb and Hubble Combine to Create Most Colorful View of Universe", "description": "This panchromatic view of galaxy cluster MACS0416 was created by combining infrared observations from NASA’s James Webb Space Telescope with visible-light data from NASA’s Hubble Space Telescope. To make the image, in general the shortest wavelengths of light were color-coded blue, the longest wavelengths red, and intermediate wavelengths green. The resulting wavelength coverage, from 0.4 to 5 microns, reveals a vivid landscape of galaxies that could be described as one of the most colorful views of the universe ever created.MACS0416 is a galaxy cluster located about 4.3 billion light-years from Earth, meaning that light we see now left the cluster shortly after the formation of our solar system. This cluster magnifies the light from more distant background galaxies through gravitational lensing. As a result, the research team has been able to identify magnified supernovae and even very highly magnified individual stars.Those colors give clues to galaxy distances: The bluest galaxies are relatively nearby and often show intense star formation, as best detected by Hubble, while the redder galaxies tend to be more distant, or else contain copious amount of dust, as detected by Webb. The image reveals a wealth of details that are only possible to capture by combining the power of both space telescopes.In this image, blue represents data at wavelengths of 0.435 and 0.606 microns (Hubble filters F435W and F606W); cyan is 0.814, 0.9, and 1.05 microns (Hubble filters F814W, and F105W and Webb filter F090W); green is 1.15, 1.25, 1.4, 1.5, and 1.6 microns (Hubble filters F125W, F140W, and F160W, and Webb filters F115W and F150W); yellow is 2.00 and 2.77 microns (Webb filters F200W, and F277W); orange is 3.56 microns (Webb filter F356W); and red represents data at 4.1 and 4.44 microns (Webb filters F410M and F444W). || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite_print.jpg (1024x949) [349.8 KB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite.png (4457x4133) [34.6 MB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite-hw.png (3840x2160) [9.6 MB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite_searchweb.png (320x180) [105.9 KB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite_thm.png (80x40) [13.0 KB] || webb-and-hubble-combine-to-create-most-colorful-view-of-universe-composite-image.hwshow [394 bytes] || ", "hits": 210 }, { "id": 14596, "url": "https://svs.gsfc.nasa.gov/14596/", "result_type": "Produced Video", "release_date": "2024-05-29T11:00:00-04:00", "title": "Lucy Sees Asteroid Dinkinesh in Detail", "description": "Narrated video of Lucy’s encounter with the main-belt asteroid Dinkinesh and its satellite, Selam, on Nov. 1, 2023.Complete transcript available.Universal Production Music: “Gaining Positivity” by Ho Ling Tang [BMI] and Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]Watch this video on the NASA Goddard YouTube channel. || Dinkinesh_Detailed_View_V2_print.jpg (1024x576) [64.4 KB] || Dinkinesh_Detailed_View_V2.jpg (1280x720) [159.2 KB] || Dinkinesh_Detailed_View_V2.png (1280x720) [165.4 KB] || Dinkinesh_Detailed_View_V2_searchweb.png (320x180) [13.4 KB] || Dinkinesh_Detailed_View_V2_thm.png (80x40) [1.9 KB] || 14596_Dinkinesh_Detailed_View_1080.mp4 (1920x1080) [55.5 MB] || 14596_Dinkinesh_Detailed_View_720.mp4 (1280x720) [11.4 MB] || DinkineshDetailedCaptions.en_US.srt [1.2 KB] || DinkineshDetailedCaptions.en_US.vtt [1.1 KB] || 14596_Dinkinesh_Detailed_View_4K.mp4 (3840x2160) [539.3 MB] || 14596_Dinkinesh_Detailed_View_ProRes.mov (3840x2160) [3.3 GB] || ", "hits": 53 }, { "id": 14581, "url": "https://svs.gsfc.nasa.gov/14581/", "result_type": "Produced Video", "release_date": "2024-05-23T10:00:00-04:00", "title": "Gliese 12 b: An Intriguing World Sized Between Earth and Venus", "description": "Gliese 12 b’s estimated size may be as large as Earth or slightly smaller — comparable to Venus in our solar system. This artist’s concept compares Earth with different possible Gliese 12 b interpretations, from no atmosphere to a thick Venus-like one. Follow-up observations with NASA’s James Webb Space Telescope will help determine just how much atmosphere the planet retains as well as its composition.Credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)Alt text: Illustration of Earth compared to various models of Gliese 12 b Image description: At left, against a black background, floats an artist's concept of a nearly half-illuminated Earth, with clouds, blue oceans, and land areas rendered in green, tan, brown, and white. At right are three similarly illuminated planets, slightly smaller than Earth and each representing a possible interpretation of Gliese 12 b. The version on the left has a surface of blotchy reddish and brownish features and no atmosphere. The middle version has the same surface texture partly obscured by a hazy atmosphere. And the rightmost and smallest version of the planet has a thick, Venus-like atmosphere that obscures the surface completely. || Gl12b_Earth_Comparison_ac.jpg (3840x2160) [935.8 KB] || Gl12b_Earth_Comparison_ac_print.jpg (1024x576) [126.0 KB] || Gl12b_Earth_Comparison.jpg (3840x2160) [929.5 KB] || Gl12b_Earth_Comparison_ac_searchweb.png (320x180) [54.4 KB] || Gl12b_Earth_Comparison_ac_web.png (320x180) [54.4 KB] || Gl12b_Earth_Comparison_ac_thm.png (80x40) [9.8 KB] || Gl12b_Earth_Comparison.tif (3840x2160) [6.4 MB] || ", "hits": 489 }, { "id": 14562, "url": "https://svs.gsfc.nasa.gov/14562/", "result_type": "Produced Video", "release_date": "2024-04-03T14:30:00-04:00", "title": "Chasing The 2024 Total Solar Eclipse With NASA Jets", "description": "The April 8, 2024, total solar eclipse will produce stunning views across North America. While anyone along the eclipse path with a clear sky will see the spectacular event, the best view might be 50,000 feet in the air, aboard NASA’s WB-57 jet planes. That’s where a trio of NASA-funded teams are sending their scientific instruments to take measurements of the eclipse.Two teams will image the Sun’s outer atmosphere – the corona – and a third will measure the ionosphere, the upper electrically charged layer of Earth’s atmosphere. This information will help scientists better understand the structure and temperature of the corona, the effects of the Sun on Earth’s atmosphere, and even aid in the search of asteroids that may orbit near the Sun. || ", "hits": 83 }, { "id": 5237, "url": "https://svs.gsfc.nasa.gov/5237/", "result_type": "Visualization", "release_date": "2024-03-29T09:00:00-04:00", "title": "Grand Average Precipitation Climatology (2000-2023)", "description": "Grand Average Precipitation Climatology ranging from June 2000 to May 2023 || IMERG_GrandAvg.jpg (4096x2048) [1.4 MB] || IMERGclim_v02_2024-03-07_1546.00002_searchweb.png (320x180) [89.6 KB] || IMERGclim_v02_2024-03-07_1546.00002_thm.png (80x40) [7.5 KB] || IMERGclim_v02_2024-03-07_1546.00002.exr (4096x2048) [18.5 MB] || ", "hits": 206 }, { "id": 14537, "url": "https://svs.gsfc.nasa.gov/14537/", "result_type": "Produced Video", "release_date": "2024-02-29T12:00:00-05:00", "title": "One Month Out From The Total Solar Eclipse Live Shots", "description": "Included on this resource page are cut broll for the live shots and pre-recorded soundbites with Gina DiBraccio / Deputy Director of Heliophysics, NASA GSFC and Nicholeen Viall / NASA Mission Scientist for PUNCH. Also check out NASA's podcast nasa.gov/curiousuniverse. New episodes coming soon including one about the April 2024 solar eclipse. || Unknown.jpeg (1600x640) [86.5 KB] || Unknown_print.jpg (1024x409) [53.1 KB] || Unknown_searchweb.png (320x180) [35.3 KB] || Unknown_thm.png (80x40) [5.1 KB] || ", "hits": 33 }, { "id": 5182, "url": "https://svs.gsfc.nasa.gov/5182/", "result_type": "Visualization", "release_date": "2024-02-02T03:00:00-05:00", "title": "50 Years of Harmful Algal Blooms: Robinson Projection", "description": "1973 - 2023 harmful algal bloom throughout the world, depicted on a Robinson projection map. || robinson_v44_2023-10-26_1326.04898_print.jpg (1024x576) [116.2 KB] || robinson_v44_2023-10-26_1326.04898_searchweb.png (320x180) [45.2 KB] || robinson_v44_2023-10-26_1326.04898_thm.png (80x40) [4.8 KB] || robinson_v44_2023-10-26_1326_1080p30.mp4 (1920x1080) [6.8 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || robinson_v44_2023-10-26_1326_1080p30.webm (1920x1080) [3.4 MB] || robinson_v44_2023-10-26_1326_1080p30.mp4.hwshow [202 bytes] || ", "hits": 144 }, { "id": 5183, "url": "https://svs.gsfc.nasa.gov/5183/", "result_type": "Visualization", "release_date": "2024-02-02T03:00:00-05:00", "title": "50 Years of Harmful Algal Blooms: Florida Zoom", "description": "50 years of global algal blooms on a rotating globe (depicted as green dots). Once all 50 years are shown, the globe continues to rotate, while the camera begins to pan up, finally zooming down to Florida. || sphere2FL_v44_2023-10-26_1330.06000_print.jpg (1024x576) [38.0 KB] || sphere2FL_v44_2023-10-26_1330.06000_searchweb.png (320x180) [19.4 KB] || sphere2FL_v44_2023-10-26_1330.06000_thm.png (80x40) [2.4 KB] || sphere2FL_v44_2023-10-26_1330.mp4 (1920x1080) [14.5 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || sphere2FL_v44_2023-10-26_1330.webm (1920x1080) [5.7 MB] || sphere2FL_v44_2023-10-26_1330.mp4.hwshow [195 bytes] || ", "hits": 32 }, { "id": 5184, "url": "https://svs.gsfc.nasa.gov/5184/", "result_type": "Visualization", "release_date": "2024-02-02T03:00:00-05:00", "title": "50 Years of Harmful Algal Blooms: Rotating Globe Unwraps to Robinson Projection", "description": "This data visualization shows 50 years of algal blooms collected across a spinning globe. Once all the data is accumulated, the globe then unwraps into a Robinson projection so the viewer can see the entire global dataset. || unwrap_v43_2023-10-26_1332.04150_print.jpg (1024x576) [63.0 KB] || unwrap_v43_2023-10-26_1332.04150_searchweb.png (320x180) [30.7 KB] || unwrap_v43_2023-10-26_1332.04150_thm.png (80x40) [3.3 KB] || unwrap_v43_2023-10-26_1332.mp4 (1920x1080) [9.5 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || unwrap_v43_2023-10-26_1332.webm (1920x1080) [3.7 MB] || unwrap_v43_2023-10-26_1332.mp4.hwshow [438 bytes] || ", "hits": 28 }, { "id": 14491, "url": "https://svs.gsfc.nasa.gov/14491/", "result_type": "Produced Video", "release_date": "2023-12-26T00:00:00-05:00", "title": "Roman Hardware Highlights", "description": "This video, covering the second half of 2025, opens with a person entering NASA’s Goddard Space Flight Center’s largest clean room, the Spacecraft Systems Development and Integration Facility. The room is a class 10,000 clean room with over one million cubic feet of space.The outside half of Roman, called OSD, contains the solar panels and protective layers. The Deployable Aperture Cover, which protects the mirrors during launch and then unfolds to help shield them from sunlight does a test deployment. During this test, lines connect to it and pull upward to negate Earth’s gravitational forces, which Roman will not experience in space. Then the Solar Array Sun Shield panels deploy. There are four panels that move. They fold against the spacecraft to fit inside the rocket fairing and then deploy in space to make a large flat plane that both collects light to generate electricity and helps keep the rest of Roman cool.In preparation for additional testing, technicians put a clean tent over OSD and transport it out of the clean room. They push it into the acoustic test chamber where a six-foot-tall horn projects up to 150-decibel sound at varying frequencies. The other tests are on two vibration tables that shake Roman along all three axes: up/down, left/right, and forward/backward. Engineers attach hundreds of sensors and run tests of increasing intensity. During and after each test, they carefully study the data to make sure that Roman is behaving as they anticipated.While these tests occur, Roman’s inside half, containing the mirrors, instruments and support equipment, move into Goddard’s largest thermal vacuum chamber, the SES (Space Environment Simulator). This 40-foot-tall chamber can simulate the vacuum of space and the wide temperature range that Roman will experience there: from -310° Fahrenheit (-190° C) to 302° Fahrenheit (150° C). The move to the chamber happens without a clean tent, so the entire path was cleaned, and all the workers dress in full clean-room garb to ensure that no dirt contaminates the sensitive parts of the spacecraft. Once the two layers of doors are sealed, Roman spends 72 days inside running through tests at various temperatures and with equipment turned on to ensure that it works at low temperature in a vacuum. A special array installed above the mirror projects light that engineers use to test the optics and sensors.After leaving the SES chamber and returning to the SSDIF, Roman’s primary and secondary mirrors are carefully cleaned and inspected. It is a balance to get the mirrors as clean as possible while not cleaning too aggressively and damaging the delicate surfaces. The mirrors are cleaned both horizontally with a gentle vacuum cleaner and vertically with brushes. After this cleaning, every inch is visually inspected and photographed to record the exact optical characteristics. This was the last time the primary mirror would be accessible.Finally, in late November, Roman’s two halves are joined together to form the complete observatory. The process takes the better part of a day. Two guide poles are installed on the inside half to help direct OSD down onto it. At various times, the clearances between the two halves are only a few inches. With the observatory complete, it begins preparing for another round of deployments and testing.Music credit: “Our Journey Begins,” Dan Thiessen [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Roman_Hardware_Highlights_SummerFall2025_3.jpg (1280x720) [473.7 KB] || Roman_HH_Summer-Fall2025_10mbps.mp4 (1920x1080) [185.0 MB] || Roman_HH_Summer-Fall2025_25mbps.mp4 (1920x1080) [452.7 MB] || Roman_HH_Summer-Fall2025_YT.mp4 (1920x1080) [880.2 MB] || RomanHHLate2025Captions.en_US.srt [588 bytes] || RomanHHLate2025Captions.en_US.vtt [570 bytes] || Roman_HH_Summer-Fall2025_ProRes_1920x1080_2997.mov (1920x1080) [2.5 GB] || ", "hits": 240 }, { "id": 5147, "url": "https://svs.gsfc.nasa.gov/5147/", "result_type": "Visualization", "release_date": "2023-09-26T17:00:00-04:00", "title": "GEOS-FP Near-Surface Temperature", "description": "Near-surface temperature is calculated by sampling 3-D atmospheric fields from NASA’s GEOS-FP system 3 meters above Earth’s surface. GEOS-FP combines millions of weather observations with a predictive model to create a global best estimate of weather conditions that are used to begin a forecast.", "hits": 101 }, { "id": 5148, "url": "https://svs.gsfc.nasa.gov/5148/", "result_type": "Visualization", "release_date": "2023-09-26T17:00:00-04:00", "title": "GEOS-FP Near-Surface Wind Speed", "description": "Near-surface wind speed is calculated by sampling 3-D atmospheric fields from NASA’s GEOS-FP system 10 meters above Earth’s surface. GEOS-FP combines millions of weather observations with a predictive model to create a global best estimate of weather conditions that are used to begin a forecast.", "hits": 114 }, { "id": 5149, "url": "https://svs.gsfc.nasa.gov/5149/", "result_type": "Visualization", "release_date": "2023-09-26T17:00:00-04:00", "title": "GEOS-FP Precipitation and Clouds", "description": "Precipitation and clouds are calculated using fields from NASA’s GEOS-FP system. GEOS-FP combines millions of weather observations with a predictive model to create a global best estimate of weather conditions, which can be used to estimate the formation of clouds along with rain and snowfall.", "hits": 89 }, { "id": 5150, "url": "https://svs.gsfc.nasa.gov/5150/", "result_type": "Visualization", "release_date": "2023-09-26T17:00:00-04:00", "title": "GEOS-FP Near-Surface Humidity", "description": "Near-surface Humidity, also known as specific humidity (Q2M) from NASA’s GEOS-FP system. GEOS-FP combines millions of weather observations with a predictive model to create a global best estimate of weather conditions that are used to begin a forecast.", "hits": 122 }, { "id": 40503, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-earth-science/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Earth Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 275 }, { "id": 5072, "url": "https://svs.gsfc.nasa.gov/5072/", "result_type": "Visualization", "release_date": "2023-07-10T15:00:00-04:00", "title": "Atlantic Hurricane Wind Speed Plots", "description": "Atlantic Hurricane season plot of time vs. wind speed. This version shows:May through Decembereach year separately || atlantic_may_to_dec.years_001_print.jpg (1024x576) [52.2 KB] || atlantic_may_to_dec.years_001_searchweb.png (320x180) [17.2 KB] || atlantic_may_to_dec.years_001.mp4 (3840x2160) [18.9 MB] || atlantic_may_to_dec.years_001 (3840x2160) [0 Item(s)] || atlantic_may_to_dec.years_001.webm (3840x2160) [4.4 MB] || ", "hits": 43 }, { "id": 14350, "url": "https://svs.gsfc.nasa.gov/14350/", "result_type": "Produced Video", "release_date": "2023-05-23T09:55:00-04:00", "title": "Hubble Hunts for Intermediate-Sized Black Hole Close to Home", "description": "Astronomers using NASA’s Hubble Space Telescope have come up with what they say is some of their best evidence yet for the presence of a rare class of “intermediate-sized” black hole that may be lurking in the heart of the closest globular star cluster to Earth, located 6,000 light-years away.Like intense gravitational potholes in the fabric of space, virtually all black holes seem to come in two sizes: small and humongous. It’s estimated that our galaxy is littered with 100 million small black holes (several times the mass of our Sun) created from exploded stars. The universe at large is flooded with supermassive black holes, weighing millions or billions of times our Sun’s mass and found in the centers of galaxies.A long-sought missing link is an intermediate-mass black hole, weighing in somewhere between 199 and 10,000 solar masses. How would they form, where would they hang out, and why do they seem to be so rare?For more information, visit https://nasa.gov/hubble. Music CreditTesseract by Cody Johnson [ASCAP] and Gina Kouyoumdjian [BMI] via Emperia Alpha Publishing [ASCAP], Emperia Beta Publishing [BMI], and Universal Production MusicAnimation Credit:Computer Representation of the Stellar Motions in the Core of M4:Mattia Libralato (AURA/STScI for ESA)Black Hole accreting material animation by Aurore Simmonet. || ", "hits": 44 }, { "id": 14351, "url": "https://svs.gsfc.nasa.gov/14351/", "result_type": "Produced Video", "release_date": "2023-05-17T00:00:00-04:00", "title": "The Science of Snow: Digging for Data", "description": "Complete transcript available. || thumbnail2.jpg (1920x1080) [643.5 KB] || thumbnail2_searchweb.png (320x180) [89.4 KB] || thumbnail2_web.png (320x180) [89.4 KB] || thumbnail2_thm.png (80x40) [7.8 KB] || SnowEx_2023_Final_Export.webm (1920x1080) [2.6 MB] || SnowEx_Transcript.mp4 [22.6 MB] || SnowEx_2023_Final_Export.mp4 (1920x1080) [1.4 GB] || ", "hits": 34 }, { "id": 5097, "url": "https://svs.gsfc.nasa.gov/5097/", "result_type": "Visualization", "release_date": "2023-04-19T00:00:00-04:00", "title": "2022 Hurricane Season", "description": "2022 Atlantic hurricane season. || hurr2022_v6.8800_print.jpg (1024x1024) [452.1 KB] || hurr2022_v6.8800_searchweb.png (320x180) [126.2 KB] || hurr2022_v6.8800_thm.png (80x40) [8.2 KB] || 2160x2160_1x1_30p (2160x2160) [0 Item(s)] || hurr2022_v6_2160p30.webm (2160x2160) [107.7 MB] || hurr2022_v6_2160p30.mp4 (2160x2160) [1.4 GB] || ", "hits": 69 }, { "id": 14287, "url": "https://svs.gsfc.nasa.gov/14287/", "result_type": "Produced Video", "release_date": "2023-03-16T14:00:00-04:00", "title": "Hubble’s Inside The Image: Crab Nebula", "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the breathtaking Crab Nebula.With an apparent magnitude of 8.4 and located 6,500 light-years from Earth in the constellation Taurus, the Crab Nebula can be spotted with a small telescope and is best observed in January. The nebula was discovered by English astronomer John Bevis in 1731, and later observed by Charles Messier who mistook it for Halley’s Comet. Messier’s observation of the nebula inspired him to create a catalog of celestial objects that might be mistaken for comets.In this video, Dr. Padi Boyd takes us on a journey through the Nebula, teaching us some of the interesting science behind this famous Hubble image.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credit:Hubble Space Telescope AnimationCredit: ESA/Hubble (M. Kornmesser & L. L. Christensen), A. Fujii, Robert Gendler, Digitized Sky Survey 2, Panther Observatory, Steve Cannistra, Michael Pierce, Robert Berrington (Indiana University), Nigel Sharp, Mark Hanna (NOAO)/WIYN/NSF. Crab Nebula Zoom VisualizationCredit: ESA/Hubble, Digitized Sky Survey, Nick Risinger (skysurvey.org) Dark Matter Gravitational Lensing AnimationCredit: NASA's Goddard Space Flight Center Conceptual Image LabMusic Credit:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Night Call” by Timothy Paul Handels [SABAM] via Pedigree Cuts [PRS] and Universal Production Music || ", "hits": 48 }, { "id": 14301, "url": "https://svs.gsfc.nasa.gov/14301/", "result_type": "Produced Video", "release_date": "2023-03-08T10:00:00-05:00", "title": "Millions of Galaxies Emerge in New Simulated Images From NASA's Roman", "description": "This video begins by showing the most distant galaxies in the simulated deep field image in red. As it zooms out, layers of nearer (yellow and white) galaxies are added to the frame. By studying different cosmic epochs, Roman will be able to trace the universe's expansion history, study how galaxies developed over time, and much more.Credit: Caltech-IPAC/R. Hurt and M. Troxel || Roman_Zoom_still.jpg (1920x1080) [515.9 KB] || Roman_Zoom_still_searchweb.png (320x180) [106.4 KB] || Roman_Zoom_still_thm.png (80x40) [6.6 KB] || Roman_Zoom-HD2K.mp4 (1920x1080) [25.3 MB] || Roman_Zoom-HD2K.webm (1920x1080) [2.7 MB] || ", "hits": 75 }, { "id": 5013, "url": "https://svs.gsfc.nasa.gov/5013/", "result_type": "Visualization", "release_date": "2022-08-19T13:00:00-04:00", "title": "Artemis III Landing Region Candidates", "description": "This narrated movie introduces Artemis III, reveals the mission's 13 candidate landing regions near the lunar South Pole, and briefly discusses some of the criteria that narrowed the selection to these regions.Music provided by Universal Production Music: Best Days to Come – Matteo Pagamici and Max Molling.This video can also be viewed on the NASA Goddard YouTube channel. || ArtemisIII_LandingRegions_print.jpg (1024x576) [130.2 KB] || ArtemisIII_LandingRegions_YouTubeHD.webm (1920x1080) [15.6 MB] || ArtemisIII_LandingRegions_YouTubeHD.mp4 (1920x1080) [230.8 MB] || ArtemisIII_LandingRegions_Captions.en_US.srt [3.0 KB] || ArtemisIII_LandingRegions_Captions.en_US.vtt [2.8 KB] || ArtemisIII_LandingRegions_MASTER.mov (1920x1080) [1.9 GB] || ", "hits": 1166 }, { "id": 14164, "url": "https://svs.gsfc.nasa.gov/14164/", "result_type": "Produced Video", "release_date": "2022-06-07T19:00:00-04:00", "title": "Australia Sounding Rocket Campaign Press Kit", "description": "NASA will launch three suborbital sounding rockets in June and July 2022 from the Arnhem Space Center in Australia’s Northern Territory to conduct astrophysics studies that can only be done from the Southern Hemisphere. The three missions will focus on α Centauri A and B, two of the three-star α Centauri system that are the closest stars to our Sun, and X-rays emanating from the interstellar medium, clouds of gases and particles between stars.The three sounding rocket night-time missions will be launched between June 26 and July 12 on two-stage Black Brant IX sounding rockets, from the Arnhem Space Center, which is owned and operated by Equatorial Launch Australia or ELA. The Arnhem Space Center is a commercial space launch facility, located on the Dhupuma Plateau near Nhulunbuy. The NASA missions will be the first launches from Arnhem.Learn more: Australia Sounding Rocket Fact SheetWatch more: Sounding Rockets: Cutting Edge Science, 15 Minutes at a TimeWhat Is a Sounding Rocket?Riding Along with a NASA Sounding Rocket || ", "hits": 67 }, { "id": 4984, "url": "https://svs.gsfc.nasa.gov/4984/", "result_type": "Visualization", "release_date": "2022-05-15T00:00:00-04:00", "title": "ICESat-2 Land Ice Height Change", "description": "At the whole ice sheet scale, this visualization shows the continued draw down of the major outlet glaciers in West Antarctica and in parts of East Antarctica between April 2019 and July 2021. Some areas show hints of blue, indicating places where the ice sheet surface has gone up, reflecting either increased snowfall or changes in ice dynamics.", "hits": 102 }, { "id": 5001, "url": "https://svs.gsfc.nasa.gov/5001/", "result_type": "Visualization", "release_date": "2022-05-05T17:00:00-04:00", "title": "Moon Mosaic", "description": "A photomosaic of the full Moon comprising 1,231 images taken by LRO's Narrow Angle Camera. || moon_mosaic_print.jpg (1024x1024) [246.6 KB] || moon_mosaic_searchweb.png (320x180) [60.0 KB] || moon_mosaic_thm.png (80x40) [13.7 KB] || moon_mosaic_big.tif (12800x12800) [72.9 MB] || moon_mosaic.tif (3200x3200) [6.2 MB] || ", "hits": 1115 }, { "id": 14148, "url": "https://svs.gsfc.nasa.gov/14148/", "result_type": "Produced Video", "release_date": "2022-05-05T12:45:00-04:00", "title": "Magnetic Flip Drives Flare-Up of Monster Black Hole", "description": "Explore the unusual eruption of 1ES 1927+654, a galaxy located 236 million light-years away in the constellation Draco. A sudden reversal of the magnetic field around its million-solar-mass black hole may have triggered the outburst.Credit: NASA’s Goddard Space Flight Center Music: \"Water Dance\" and \"Alternate Worlds\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || ChangingLookAGN_Still1.jpg (1920x1080) [822.9 KB] || ChangingLookAGN_Still1_searchweb.png (320x180) [79.5 KB] || ChangingLookAGN_Still1_thm.png (80x40) [6.2 KB] || 14148_ChangingLook_AGN_1080.webm (1920x1080) [24.8 MB] || 14148_ChangingLook_AGN_Sub100MB.mp4 (1920x1080) [91.5 MB] || 14148_ChangingLook_AGN_1080.mp4 (1920x1080) [246.5 MB] || 14148_ChangingLook_AGN_Best_1080.mp4 (1920x1080) [534.7 MB] || 14148_ChangingLook_AGN_SRT_Captions.en_US.srt [4.2 KB] || 14148_ChangingLook_AGN_SRT_Captions.en_US.vtt [4.3 KB] || 14148_ChangingLook_AGN_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ", "hits": 247 }, { "id": 14149, "url": "https://svs.gsfc.nasa.gov/14149/", "result_type": "Produced Video", "release_date": "2022-05-02T10:45:00-04:00", "title": "NASA's Black Hole Orrery", "description": "Learn more about the best-known black hole systems in our galaxy and its neighbor, the Large Magellanic Cloud. This visualization presents 22 X-ray binary systems that host confirmed black holes at the same scale, with their orbits sped up by about 22,000 times. The view of each system reflects how we see it from Earth. Star colors ranging from blue-white to reddish represent temperatures from 5 times hotter to 45% cooler than our Sun. In most of these systems, a stream of matter from the star forms an accretion disk around the black hole. In others, like the famous system called Cygnus X-1, the star produces a hefty outflow that is partly swept up by the black hole’s gravity to form the disk. The accretion disks use a different color scheme because they sport even higher temperatures than the stars. The largest disk shown, belonging to a binary called GRS 1915, spans a distance greater than that separating Mercury from our Sun. The black holes themselves are shown larger than in reality using spheres scaled to reflect their masses.Credit: NASA's Goddard Space Flight Center and Scientific Visualization StudioMusic: \"Event Horizon\" from Gravity. Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Black_Hole_Orrery_Still.jpg (3840x2160) [321.9 KB] || Black_Hole_Orrery_Still_searchweb.png (320x180) [25.6 KB] || Black_Hole_Orrery_Still_thm.png (80x40) [4.1 KB] || 14149_Black_Hole_Orrery_FINAL_1080.mp4 (1920x1080) [118.8 MB] || 14149_Black_Hole_Orrery_FINAL_1080.webm (1920x1080) [12.4 MB] || 14149_Black_Hole_Orrery_ProRes_3840x2160_2997.mov (3840x2160) [1.9 GB] || 14149_Black_Hole_Orrery_FINAL_4k_Best.mp4 (3840x2160) [379.2 MB] || 14149_Black_Hole_Orrery_FINAL_4k.mp4 (3840x2160) [176.7 MB] || 14149_Black_Hole_Orrery_SRT_Captions.en_US.srt [1.9 KB] || 14149_Black_Hole_Orrery_SRT_Captions.en_US.vtt [1.9 KB] || ", "hits": 236 }, { "id": 4982, "url": "https://svs.gsfc.nasa.gov/4982/", "result_type": "Visualization", "release_date": "2022-04-21T09:00:00-04:00", "title": "Complete 2021 Hurricane Season", "description": "This special version of the 2021 Hurricane Season data visualization uses all the below layers to show the entire 2021 Hurricane Season, but elements of it were sped up in post production to accelerate the data when no hurricanes are present. This provides the viewer with a more compact experience that focuses exclusively on the hurricanes. || hurr2021_comp5speed_2160p30.04733_print.jpg (1024x576) [248.6 KB] || hurr2021_speedComp7_1080p30.mp4 (1920x1080) [437.0 MB] || Sample_Speed_Composite (3840x2160) [0 Item(s)] || hurr2021_speedComp7.webm (3840x2160) [91.3 MB] || hurr2021_speedComp7.mp4 (3840x2160) [197.5 MB] || ", "hits": 87 }, { "id": 14133, "url": "https://svs.gsfc.nasa.gov/14133/", "result_type": "Produced Video", "release_date": "2022-04-06T13:00:00-04:00", "title": "Concert videos", "description": "These videos are designed to accompany live orchestral performances. For more information and inquiries about their use, please contact Scott Wiessinger at scott.wiessinger@nasa.gov. || ", "hits": 49 }, { "id": 31180, "url": "https://svs.gsfc.nasa.gov/31180/", "result_type": "Hyperwall Visual", "release_date": "2022-03-10T10:00:00-05:00", "title": "NASA and Agriculture: From Seeds to Satellites", "description": "Complete transcript available. || ComClas_Final_Cut.00148_print.jpg (1024x576) [55.5 KB] || Screen_Shot_2022-03-03_at_1.29.01_PM.png (2478x1382) [1.5 MB] || ComClas_Final_Cut.00148_searchweb.png (320x180) [45.5 KB] || ComClas_Final_Cut.00148_web.png (320x180) [45.5 KB] || ComClas_Final_Cut.00148_thm.png (80x40) [4.1 KB] || ComClas_Final_Cut.webm (1920x1080) [8.0 MB] || ComClas_Final_Cut.mp4 (1920x1080) [126.1 MB] || ComClas_Final_Cut_otter_ai.en_US.srt [1009 bytes] || ComClas_Final_Cut_otter_ai.en_US.vtt [1022 bytes] || ", "hits": 205 }, { "id": 14115, "url": "https://svs.gsfc.nasa.gov/14115/", "result_type": "Produced Video", "release_date": "2022-03-08T13:00:00-05:00", "title": "NASA's NICER Tracks a Magnetar's Hot Spots", "description": "Explore how NASA’s Neutron star Interior Composition Explorer (NICER) tracked brilliant hot spots on the surface of an erupting magnetar – from 13,000 light-years away. Credit: NASA's Goddard Space Flight CenterMusic: \"Particles and Fields\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Magnetar_Still.jpg (1920x1080) [574.3 KB] || Magnetar_Still_print.jpg (1024x576) [229.0 KB] || Magnetar_Still_searchweb.png (320x180) [66.1 KB] || Magnetar_Still_thm.png (80x40) [5.2 KB] || 14115_Merging_Magnetar_HotSpots_1080_Best.webm (1920x1080) [17.4 MB] || 14115_Merging_Magnetar_HotSpots_1080.mp4 (1920x1080) [158.9 MB] || 14115_Merging_Magnetar_HotSpots_1080_Best.mp4 (1920x1080) [382.0 MB] || 14115_Migrating_Magnetar_HotSpots_1080.en_US.srt [2.1 KB] || 14115_Migrating_Magnetar_HotSpots_1080.en_US.vtt [2.1 KB] || 14115_Merging_Magnetar_HotSpots_ProRes_1920x1080_2997.mov (1920x1080) [2.1 GB] || ", "hits": 202 }, { "id": 4974, "url": "https://svs.gsfc.nasa.gov/4974/", "result_type": "Visualization", "release_date": "2022-03-02T13:00:00-05:00", "title": "Impact of Climate Change on Global Agricultural Yields", "description": "Data visualization of predicted wheat and maize yields through the end of this centaury based on an ensemble of crop and climate models. || AgMapMaize.00900_print.jpg (1024x576) [125.5 KB] || AgMapMaize.00900_searchweb.png (180x320) [54.2 KB] || AgMapMaize.00900_thm.png (80x40) [5.7 KB] || AgMapMaize.mp4 (3840x2160) [48.0 MB] || maize (3840x2160) [0 Item(s)] || AgMapMaize.webm (3840x2160) [5.7 MB] || ", "hits": 755 }, { "id": 14099, "url": "https://svs.gsfc.nasa.gov/14099/", "result_type": "Produced Video", "release_date": "2022-02-28T00:00:00-05:00", "title": "Black Hole Week Assets", "description": "This page will introduce you to the world, characters, colors, and fonts of Black Hole Week. NASA celebrated Black Hole Week in 2019, 2021 and May, 2022.The world of Black Hole Week is bold, colorful, and a bit retro. It's also populated by a fun bunch of characters, including a little blue explorer (called the \"Traveler\") and their black hole friends. Below, you'll find tons of helpful images, GIFs, and other materials to get you going if you want to join in!If you are having trouble downloading the ZIP or AI files, please contact Barb Mattson: barb.mattson@nasa.gov || ", "hits": 157 }, { "id": 14098, "url": "https://svs.gsfc.nasa.gov/14098/", "result_type": "Produced Video", "release_date": "2022-02-10T10:30:00-05:00", "title": "IMPACTS 2022: NASA Planes Fly into Snowstorms to Study Snowfall", "description": "NASA’s Investigation of Microphysics and Precipitation for Atlantic Coast-Threatening Storms (IMPACTS) mission, which began in January and is planned to wrap up at the end of February, has seen upwards of 10 flights so far. Ultimately, what the IMPACTS team learns about snowstorms will improve meteorological models and our ability to use satellite data to predict how much snow will fall and where.Music credit: “Struggles” and “Natural Time Cycles” from Universal Production MusicComplete transcript available. || Thumbnail.jpg (1920x1080) [737.2 KB] || Thumbnail_print.jpg (1024x576) [275.6 KB] || Thumbnail_searchweb.png (320x180) [100.7 KB] || IMPACTS_Final_Cut.webm (1920x1080) [21.1 MB] || IMPACTS_Final_Cut.mp4 (1920x1080) [378.3 MB] || IMPACTS_Final_1_otter_ai.en_US.srt [3.2 KB] || IMPACTS_Final_1_otter_ai.en_US.vtt [3.2 KB] || ", "hits": 26 }, { "id": 14004, "url": "https://svs.gsfc.nasa.gov/14004/", "result_type": "Produced Video", "release_date": "2021-11-17T00:00:00-05:00", "title": "Elements of Webb: Gold Part 2 Ep02", "description": "Elements of Webb EP02: Gold Part Two || 2-Gold_2_-_Dark.jpg (1920x1080) [1.1 MB] || 2-Gold_2_-_Dark_print.jpg (1024x576) [473.1 KB] || 2-Gold_2_-_Dark_searchweb.png (320x180) [100.6 KB] || 2-Gold_2_-_Dark_web.png (320x180) [100.6 KB] || 2-Gold_2_-_Dark_thm.png (80x40) [7.5 KB] || 2-Elements_-_Gold_2.webm (1920x1080) [34.9 MB] || 2-Elements_-_Gold_2.en_US.srt [5.8 KB] || 2-Elements_-_Gold_2.en_US.vtt [5.8 KB] || 2-Elements_-_Gold_2_ProRes.mov (1920x1080) [4.2 GB] || 2-Elements_-_Gold_2.mp4 (1920x1080) [324.5 MB] || elements-of-webb-gold-part-2-ep02.hwshow [293 bytes] || ", "hits": 31 }, { "id": 14003, "url": "https://svs.gsfc.nasa.gov/14003/", "result_type": "Produced Video", "release_date": "2021-11-10T00:00:00-05:00", "title": "Elements of Webb: Gold Part 1 Ep01", "description": "Elements of Webb EP01: Gold Part One || 1-Gold_1_-_Dark.jpg (1920x1080) [958.4 KB] || 1-Gold_1_-_Dark_print.jpg (1024x576) [388.7 KB] || 1-Gold_1_-_Dark_searchweb.png (320x180) [90.4 KB] || 1-Gold_1_-_Dark_web.png (320x180) [90.4 KB] || 1-Gold_1_-_Dark_thm.png (80x40) [7.4 KB] || 1-Elements-_Gold_1.webm (1920x1080) [25.6 MB] || 1-Elements-_Gold_1.en_US.srt [4.1 KB] || 1-Elements-_Gold_1_ProRes.mov (1920x1080) [3.2 GB] || 1-Elements-_Gold_1.mp4 (1920x1080) [239.5 MB] || elements-of-webb-gold-part-1-ep01.hwshow [291 bytes] || ", "hits": 25 }, { "id": 4947, "url": "https://svs.gsfc.nasa.gov/4947/", "result_type": "Visualization", "release_date": "2021-10-30T00:00:00-04:00", "title": "2021 Hurricane Season through September", "description": "This data visualization shows hurricane tracks over clouds over precipitation over sea surface temperatures from May 1 through September 30th, 2021. This presentation was created for the COP 26 Conference. || hurr2021_4k_comp.4991_print.jpg (1024x576) [337.4 KB] || hurr2021_4k_comp.4991_searchweb.png (320x180) [123.6 KB] || hurr2021_4k_comp.4991_thm.png (80x40) [17.6 KB] || hurr2021_comp_1080p30.webm (1920x1080) [29.0 MB] || hurr2021_comp_1080p30.mp4 (1920x1080) [489.6 MB] || composite (3840x2160) [0 Item(s)] || hurr2021_comp_2160p30.mp4 (3840x2160) [1.7 GB] || hurr2021_comp_1080p30.mp4.hwshow [187 bytes] || ", "hits": 55 }, { "id": 4914, "url": "https://svs.gsfc.nasa.gov/4914/", "result_type": "Visualization", "release_date": "2021-09-01T00:00:00-04:00", "title": "Impact of Climate Change on Global Wheat Yields", "description": "Data visualization of predicted Wheat yields through the end of this centaury based on an ensemble of crop and climate models. || WheatMapFuture.01000_print.jpg (1024x576) [123.1 KB] || WheatMapFuture.01000_searchweb.png (320x180) [54.6 KB] || WheatMapFuture.01000_web.png (320x180) [54.6 KB] || WheatMapFuture.01000_thm.png (80x40) [5.4 KB] || WheatMapFuture_1080p.mp4 (1920x1080) [21.7 MB] || WheatMapFuture.mp4 (3840x2160) [79.7 MB] || WheatMapFuture.webm (3840x2160) [6.4 MB] ||", "hits": 126 }, { "id": 13887, "url": "https://svs.gsfc.nasa.gov/13887/", "result_type": "Produced Video", "release_date": "2021-07-27T10:00:00-04:00", "title": "DAVINCI Probe's Eye View", "description": "An overview of the DAVINCI mission through the eyes of the descent probe.Music is \"Mountains of Hokkaido\" by Natalie Holt and Yoann Le Dantec of Universal Production Music || 13887_DAVINCI_PEVAA.02257_print.jpg (1024x576) [101.1 KB] || 13887_thumbnail.jpg (1920x1080) [157.6 KB] || 13887_DAVINCI_PEVAA.02257_searchweb.png (320x180) [69.3 KB] || 13887_DAVINCI_PEVAA.02257_thm.png (80x40) [5.1 KB] || 13887_DAVINCI_PEVAA.mp4 (1920x1080) [177.3 MB] || 13887_DAVINCI_PEVAA_twitter_720.mp4 (1280x720) [32.7 MB] || 13887_DAVINCI_PEVAA_facebook_720.mp4 (1280x720) [190.4 MB] || 13887_DAVINCI_PEVAA.webm (960x540) [47.1 MB] || 13877_DAVINCI_PEVAA_caption.en_US.srt [2.9 KB] || 13877_DAVINCI_PEVAA_caption.en_US.vtt [2.8 KB] || ", "hits": 84 }, { "id": 4903, "url": "https://svs.gsfc.nasa.gov/4903/", "result_type": "Visualization", "release_date": "2021-04-26T09:00:00-04:00", "title": "May 26, 2021 Total Lunar Eclipse: Shadow View", "description": "Pacific Daylight Time (PDT). The Moon moves right to left, passing through the penumbra and umbra, leaving in its wake an eclipse diagram with the times at various stages of the eclipse. || pdt_print.jpg (1024x576) [72.9 KB] || pdt_searchweb.png (320x180) [45.2 KB] || pdt_thm.png (80x40) [4.9 KB] || eclipse_202105_pdt_1080p30.mp4 (1920x1080) [8.4 MB] || eclipse_202105_pdt_720p30.mp4 (1280x720) [4.6 MB] || fancy_pdt (1920x1080) [0 Item(s)] || eclipse_202105_pdt_720p30.webm (1280x720) [7.8 MB] || eclipse_202105_pdt_2160p30.mp4 (3840x2160) [26.3 MB] || eclipse_202105_pdt_360p30.mp4 (640x360) [1.7 MB] || fancy_pdt (3840x2160) [0 Item(s)] || eclipse_202105_pdt_1080p30.mp4.hwshow [192 bytes] || ", "hits": 76 }, { "id": 13828, "url": "https://svs.gsfc.nasa.gov/13828/", "result_type": "Produced Video", "release_date": "2021-04-06T16:00:00-04:00", "title": "Welcome to the Next Wright Brothers Moment: NASA Ingenuity Helicopter Days Away From First Test Flight on Mars Live Shots", "description": "Click here for link to Ingenuity press kit. Includes information and links to b-roll.Check out raw images from the Mars Perseverance Rover here.Make your own paper Mars helicopter!Perseverance took a SELFIE with Ingenuity!Check out the CLOSE UP of Ingenuity || Unknown.png (6664x1667) [3.0 MB] || Unknown_print.jpg (1024x256) [50.9 KB] || Unknown_searchweb.png (320x180) [37.5 KB] || Unknown_thm.png (80x40) [4.2 KB] || ", "hits": 55 }, { "id": 13806, "url": "https://svs.gsfc.nasa.gov/13806/", "result_type": "Produced Video", "release_date": "2021-03-12T11:00:00-05:00", "title": "Scientists Build a Detailed Image of U Mon Binary", "description": "Two stars orbit each other within an enormous dusty disk in the U Monocerotis system, illustrated here. When the stars are farthest from each other, they funnel material from the disk’s inner edge. At this time, the primary star is slightly obscured by the disk from our perspective. The primary star, a yellow supergiant, expands and contracts. The smaller secondary star is thought to maintain its own disk of material, which likely powers an outflow of gas that emits X-rays.This listing includes Spanish-language and music-free versions.Credit: NASA’s Goddard Space Flight Center/Chris Smith (USRA/GESTAR)Music: \"Moving in Thought\" from Universal Production MusicNote: While this video in its entirety can be shared without permission, its music has been licensed and may not be excised or remixed in other products. || u_mon_full_edit_still.jpg (1920x1080) [707.8 KB] || u_mon_full_edit_still_print.jpg (1024x576) [294.6 KB] || u_mon_full_edit_still_searchweb.png (320x180) [80.8 KB] || u_mon_full_edit_still_web.png (320x180) [80.8 KB] || u_mon_full_edit_still_thm.png (80x40) [6.4 KB] || u_mon_full_edit_w_music_spanish_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_HQ.mp4 (1920x1080) [90.3 MB] || u_mon_full_edit_w_music_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_w_music_SVS_preview.webm (1280x720) [5.5 MB] || u_mon_full_edit_w_music_spanish_prores.mov (1920x1080) [526.2 MB] || u_mon_full_edit_w_music_spanish_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_w_music_prores.mov (1920x1080) [526.5 MB] || u_mon_full_edit_w_music_SVS_preview.mp4 (1280x720) [30.0 MB] || u_mon_full_edit_w_music_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_spanish_prores.mov (1920x1080) [488.5 MB] || u_mon_full_edit_prores.mov (1920x1080) [488.8 MB] || u_mon_full_edit_LQ.mp4 (1920x1080) [48.6 MB] || u_mon_full_edit_captions.en_US.vtt [536 bytes] || u_mon_full_edit_captions.en_US.srt [581 bytes] || ", "hits": 28 }, { "id": 13823, "url": "https://svs.gsfc.nasa.gov/13823/", "result_type": "Produced Video", "release_date": "2021-03-03T09:55:00-05:00", "title": "Hubble Celebrates World Wildlife Day", "description": "To celebrate 2021's World Wildlife Day, the Hubble Space Telescope wanted to share all of the best \"animal\" images taken over the years. From giant tadpole galaxies to the famed Eagle Nebula, there are all kinds of \"animals\" in space!For more information, visit https://nasa.gov/hubble.Image Credits:Picture of Eagle by Eliot MalumuthPicture of Horse by Maria Zubareva via Motion ArrayVideo Credits:White Mouse in Hands by Misharin via Motion ArraySand Crab Scavenging via monster/Pond5Underwater Frog Tadpole via MPS_Images/Pond5Whale in Ocean via VideoFort/Pond5Music Credits:“Fröhlicher Bummler” by Conny Schumann [GEMA], via Ed. Beco Tapes [GEMA] and Universal Production Music || ", "hits": 29 }, { "id": 4884, "url": "https://svs.gsfc.nasa.gov/4884/", "result_type": "Visualization", "release_date": "2021-02-25T03:00:00-05:00", "title": "2020 Hurricane Season", "description": "Data visualization of the 2020 Hurricane Season. Starts on May 1, 2020 just showing Sea Surface Temperatures and cloud cover. Precipitation data then dissolves in as hurricanes are tracked throughout 2020. Hurricane tracks include Hurricane strengths depicted with the letter \"T\" for Tropical Storm and numbers for each storm's respective strength. The visualization then culminates by showing all the storm tracks at once.This video is also available on our YouTube channel. || hurr2020_4k_comp.7968_print.jpg (1024x576) [248.0 KB] || hurr2020_4k_comp.7968_searchweb.png (320x180) [93.7 KB] || hurr2020_4k_comp.7968_thm.png (80x40) [7.3 KB] || Example_Composite (1920x1080) [0 Item(s)] || hurr2020_comp_1080p30.mp4 (1920x1080) [637.6 MB] || Example_Composite (3840x2160) [0 Item(s)] || captions_silent.30824.en_US.srt [43 bytes] || hurr2020_4k_comp_2160p30.webm (3840x2160) [167.6 MB] || hurr2020_4k_comp_2160p30.mp4 (3840x2160) [1.6 GB] || hurr2020_comp_1080p30.mp4.hwshow [187 bytes] || ", "hits": 78 }, { "id": 13795, "url": "https://svs.gsfc.nasa.gov/13795/", "result_type": "Produced Video", "release_date": "2021-01-25T10:00:00-05:00", "title": "NASA’s Roman Mission Will Probe Galaxy’s Core for Hot Jupiters, Brown Dwarfs", "description": "Illustration depicting a brown dwarf, which range from about 4,000 to 25,000 times Earth’s mass. They’re too heavy to be characterized as planets, but not quite massive enough to undergo nuclear fusion in their cores like stars. Watch this video on the NASA.gov Video YouTube channel. || Brown_Dwarf_Still.png (1920x1080) [2.0 MB] || Brown_Dwarf_Still.jpg (1920x1080) [742.2 KB] || Brown_Dwarf_Still_print.jpg (1024x576) [116.6 KB] || Brown_Dwarf_Still_searchweb.png (320x180) [63.0 KB] || Brown_Dwarf_Still_thm.png (80x40) [3.6 KB] || Brown_Dwarf_Beauty_Pass_1080.mp4 (1920x1080) [37.5 MB] || Brown_Dwarf_Beauty_Pass_1080.webm (1920x1080) [2.3 MB] || Brown_Dwarf_Beauty_Pass_ProRes_3840x2160.mov (3840x2160) [1.4 GB] || Brown_Dwarf_Beauty_Pass_4k.mp4 (3840x2160) [101.5 MB] || ", "hits": 64 }, { "id": 13792, "url": "https://svs.gsfc.nasa.gov/13792/", "result_type": "Produced Video", "release_date": "2021-01-13T12:15:00-05:00", "title": "NASA Missions Unveil Magnetar Eruptions in Nearby Galaxies", "description": "On April 15, 2020, a wave of X-rays and gamma rays lasting only a fraction of a second triggered detectors on NASA and European spacecraft. The event was a giant flare from a magnetar, a type of city-sized stellar remnant that boasts the strongest magnetic fields known. Watch to learn more.Credit: NASA’s Goddard Space Flight CenterMusic: \"Collision Course-Alternative Version\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || MGF_Video_Still.jpg (1920x1080) [602.3 KB] || MGF_Video_Still_print.jpg (1024x576) [264.7 KB] || MGF_Video_Still_searchweb.png (320x180) [74.9 KB] || MGF_Video_Still_thm.png (80x40) [5.7 KB] || 13792_Magnetar_Giant_Flare_ProRes_1920x1080_2997.mov (1920x1080) [2.6 GB] || 13792_Magnetar_Giant_Flare_best_1080.mp4 (1920x1080) [498.6 MB] || 13792_Magnetar_Giant_Flare_good_1080.mp4 (1920x1080) [221.6 MB] || 13792_Magnetar_Giant_Flare_best_1080.webm (1920x1080) [24.0 MB] || 13792_Magnetar_Giant_Flare_SRT_Captions.en_US.srt [4.0 KB] || 13792_Magnetar_Giant_Flare_SRT_Captions.en_US.vtt [4.0 KB] || ", "hits": 227 }, { "id": 13764, "url": "https://svs.gsfc.nasa.gov/13764/", "result_type": "Produced Video", "release_date": "2020-12-03T06:00:00-05:00", "title": "Hubble Wraps Its 30th Year with Dazzling New Images Live Shots", "description": "** CLICK HERE FOR NEW CALDWELL IMAGE COLLECTION **** QUICK LINK TO NEW IMAGES ROLL-INS. **QUICK LINK TO ROLL-INS FOR THE LIVE SHOTS.Click here for more about the Hubble Space Telescope. Follow us on social media @NASAHubble to grab a front row seat to the universe.For the full collection of Hubble videos please see this Gallery page. || General_Advisory_Banner.png (6250x2085) [1.9 MB] || General_Advisory_Banner_print.jpg (1024x341) [86.9 KB] || General_Advisory_Banner_searchweb.png (320x180) [88.4 KB] || General_Advisory_Banner_thm.png (80x40) [6.7 KB] || ", "hits": 106 }, { "id": 13734, "url": "https://svs.gsfc.nasa.gov/13734/", "result_type": "Produced Video", "release_date": "2020-11-17T09:45:00-05:00", "title": "Technology Meets Conservation", "description": "In a constantly changing world, the protection of our planet’s endangered species and ecosystems is a priority for ecologists. Recently, a group of researchers at the University of Idaho have worked to combine their extensive on-the-ground research of the endangered Yuma Ridgway’s rail with Landsat’s vast archive, to create a habitat suitability model that can be used by land managers. By using this model, it gives land managers the tools and data to make decisions of how to best carry out conservation for the Yuma Ridgway’s rail on a year to year basis. With the success of this initial model, it’s hypothesized that this tool will be able to help additional species in the area and others down the road.To view the map, click https://sites.google.com/view/habitatsuitability-yrr/homeThe Landsat Program is a series of Earth-observing satellite missions jointly managed by NASA and the U.S. Geological Survey (USGS). Landsat satellites have been consistently gathering data about our planet since 1972. They continue to improve and expand this unparalleled record of Earth's changing landscapes for the benefit of all. || ", "hits": 22 }, { "id": 4868, "url": "https://svs.gsfc.nasa.gov/4868/", "result_type": "Visualization", "release_date": "2020-10-26T09:00:00-04:00", "title": "The Moon's Clavius Crater", "description": "A slow flyover of Clavius crater, looking south. || clavius.1800_print.jpg (1024x576) [146.9 KB] || clavius.1800_searchweb.png (320x180) [90.6 KB] || clavius.1800_thm.png (80x40) [6.7 KB] || clavius_1080p60.mp4 (1920x1080) [24.0 MB] || clavius_720p60.mp4 (1280x720) [11.3 MB] || clavius_1080p30.mp4 (1920x1080) [21.3 MB] || clavius_720p30.mp4 (1280x720) [19.7 MB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || clavius_720p30.webm (1280x720) [7.3 MB] || clavius_360p60.mp4 (640x360) [4.5 MB] || clavius_360p30.mp4 (640x360) [7.6 MB] || clavius_1080p60.mov (1920x1080) [1.2 GB] || clavius_1080p30.mp4.hwshow [181 bytes] || ", "hits": 833 }, { "id": 13721, "url": "https://svs.gsfc.nasa.gov/13721/", "result_type": "Produced Video", "release_date": "2020-09-22T11:45:00-04:00", "title": "International Observe the Moon Night live shots", "description": "Quick link to associated B-ROLL for interviews.Quick link to canned interview with Andrea Jones NASA Public Engagement / Director, International Observe the Moon NightClick here to find out more about this year's International Observe the Moon night || observe-moon-night.png (1920x1080) [552.9 KB] || observe-moon-night_print.jpg (1024x576) [71.6 KB] || observe-moon-night_searchweb.png (320x180) [47.3 KB] || observe-moon-night_thm.png (80x40) [5.2 KB] || ", "hits": 102 }, { "id": 13628, "url": "https://svs.gsfc.nasa.gov/13628/", "result_type": "Produced Video", "release_date": "2020-06-12T10:00:00-04:00", "title": "Parker Solar Probe Teams Up with Observatories Around the Solar System for Fourth Solar Encounter", "description": "At the heart of understanding our space environment is the knowledge that conditions throughout space — from the Sun to the atmospheres of planets to the radiation environment in deep space — are connected.Studying this connection – a field of science called heliophysics — is a complex task: Researchers track sudden eruptions of material, radiation, and particles against the background of the ubiquitous outflow of solar material.A confluence of events in early 2020 created a nearly ideal space-based laboratory, combining the alignment of some of humanity’s best observatories — including Parker Solar Probe, during its fourth solar flyby — with a quiet period in the Sun’s activity, when it’s easiest to study those background conditions. These conditions provided a unique opportunity for scientists to study how the Sun influences conditions at points throughout space, with multiple angles of observation and at different distances from the Sun. || ", "hits": 67 }, { "id": 40413, "url": "https://svs.gsfc.nasa.gov/gallery/earth-science-playlist/", "result_type": "Gallery", "release_date": "2020-04-01T00:00:00-04:00", "title": "Earth Science Playlist", "description": "No description available.", "hits": 10 }, { "id": 20315, "url": "https://svs.gsfc.nasa.gov/20315/", "result_type": "Animation", "release_date": "2020-03-30T10:00:00-04:00", "title": "Roman Space Telescope Microlensing Animations", "description": "This animation illustrates the concept of gravitational microlensing. When one star in the sky appears to pass nearly in front of another, the light rays of the background source star become bent due to the warped space-time around the foreground star. This star is then a virtual magnifying glass, amplifying the brightness of the background source star, so we refer to the foreground star as the lens star. If the lens star harbors a planetary system, then those planets can also act as lenses, each one producing a short deviation in the brightness of the source. Thus we discover the presence of exoplanets, and measure its mass and separation from its star. Credit: NASA's Goddard Space Flight Center/CI LabWatch this video on the NASA.gov Video YouTube channel. || WFIRST_Microlensing_S1a_4k_30fps_ProRes.00236_print.jpg (1024x576) [57.6 KB] || WFIRST_Microlensing_S1a_4k_30fps_ProRes.mov (3840x2160) [1.9 GB] || WFIRST_Microlensing_S1a_4k_30fps_h264.mp4 (3840x2160) [20.7 MB] || S1a (3840x2160) [64.0 KB] || WFIRST_Microlensing_S1a_4k_30fps_h264.webm (3840x2160) [2.9 MB] || ", "hits": 143 }, { "id": 31106, "url": "https://svs.gsfc.nasa.gov/31106/", "result_type": "Hyperwall Visual", "release_date": "2020-02-12T00:00:00-05:00", "title": "Fires Light Up Mount Vesuvius", "description": "Wildfires on Mount Vesuvius || volcano-vesuvius_print.jpg (1024x576) [98.9 KB] || volcano-vesuvius.png (3840x2160) [3.5 MB] || volcano-vesuvius_searchweb.png (320x180) [66.4 KB] || volcano-vesuvius_thm.png (80x40) [5.3 KB] || fires-light-up-mount-vesuvius.hwshow [285 bytes] || ", "hits": 28 }, { "id": 13534, "url": "https://svs.gsfc.nasa.gov/13534/", "result_type": "Produced Video", "release_date": "2020-01-31T16:00:00-05:00", "title": "The Countdown is on for Launch of NASA’s Next Mission to Face the Sun Live Shots", "description": "B-roll and canned interviews will be added by Thursday at 4:00 p.m. ESTSolar Orbiter Will Give Humanity Its First Close-Up Look At The Sun’s Poles || screengrab.png (2306x724) [2.8 MB] || screengrab_print.jpg (1024x321) [99.4 KB] || screengrab_searchweb.png (320x180) [126.2 KB] || screengrab_thm.png (80x40) [8.4 KB] || ", "hits": 44 }, { "id": 40409, "url": "https://svs.gsfc.nasa.gov/gallery/fermi-stills/", "result_type": "Gallery", "release_date": "2020-01-22T00:00:00-05:00", "title": "Fermi Stills", "description": "A collection of Fermi-related still images, illustrations, graphics and short clips.", "hits": 277 }, { "id": 13513, "url": "https://svs.gsfc.nasa.gov/13513/", "result_type": "Produced Video", "release_date": "2019-12-23T10:00:00-05:00", "title": "The Best Gift of All: A Box of Moon Soil", "description": "Jamie Elsila and Danielle Simkus prepare previously unopened Apollo 17 Moon samples for analysis. Music is \"Fairy Christmas\" from Universal Production Music. || 13513_THUMBNAIL.jpg (1920x1080) [672.4 KB] || 13513_ApolloSampleGift_MASTER.00576_searchweb.png (320x180) [91.6 KB] || 13513_ApolloSampleGift_MASTER.00576_thm.png (80x40) [7.1 KB] || 13513_ApolloSampleGift_MASTER.mov (1920x1080) [1.1 GB] || 13513_ApolloSampleGift_MASTER_facebook_720.mp4 (1280x720) [115.9 MB] || 13513_ApolloSampleGift_MASTER_twitter_720.mp4 (1280x720) [20.1 MB] || 13513_ApolloSampleGift_MASTER.webm (960x540) [38.3 MB] || 13513_Apollo.en_US.srt [772 bytes] || 13513_Apollo.en_US.vtt [788 bytes] || ", "hits": 61 }, { "id": 13209, "url": "https://svs.gsfc.nasa.gov/13209/", "result_type": "Produced Video", "release_date": "2019-12-19T12:00:00-05:00", "title": "NASA’s Fermi Finds Vast ‘Halo’ Around Nearby Pulsar", "description": "Astronomers using data from NASA’s Fermi mission have discovered a pulsar with a faint gamma-ray glow that spans a huge part of the sky. Watch to learn more.Credit: NASA’s Goddard Space Flight CenterMusic: \"Insight\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Geminga_Still.jpg (1920x1080) [177.1 KB] || Geminga_Still_print.jpg (1024x576) [65.2 KB] || Geminga_Still_searchweb.png (320x180) [75.1 KB] || Geminga_Still_thm.png (80x40) [5.6 KB] || 13209_Fermi_Geminga_Halo_ProRes_1920x1080_2997.mov (1920x1080) [1.7 GB] || 13209_Fermi_Geminga_Halo_1080_Best.mp4 (1920x1080) [294.5 MB] || 13209_Fermi_Geminga_Halo_1080_Best.webm (1920x1080) [15.3 MB] || 13209_Fermi_Geminga_Halo_1080_Good.mp4 (1920x1080) [144.1 MB] || Fermi_Geminga_Halo_SRT_Captions.en_US.srt [1.7 KB] || Fermi_Geminga_Halo_SRT_Captions.en_US.vtt [1.7 KB] || ", "hits": 76 }, { "id": 13240, "url": "https://svs.gsfc.nasa.gov/13240/", "result_type": "Produced Video", "release_date": "2019-12-12T11:00:00-05:00", "title": "NASA’s NICER Sizes Up a Pulsar, Reveals First-ever Surface Map", "description": "Watch how NASA’s Neutron star Interior Composition Explorer (NICER) has expanded our understanding of pulsars, the dense, spinning corpses of exploded stars. Pulsar J0030+0451 (J0030 for short), located 1,100 light-years away in the constellation Pisces, now has the most precise and reliable measurements of both a pulsar’s mass and size to date. The shapes and locations of its hot spots challenge textbook depictions of these incredible objects. Music: \"Uncertain Ahead\" and \"Flowing Cityscape\" (underscore). Both from Universal Production MusicCredit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Two_NS_Model_Still.jpg (1920x1080) [308.5 KB] || Two_NS_Model_Still_print.jpg (1024x576) [140.4 KB] || Two_NS_Model_Still_searchweb.png (320x180) [87.0 KB] || Two_NS_Model_Still_thm.png (80x40) [8.0 KB] || 13240_NICER_J0030_MassRadius_1080.webm (1920x1080) [33.5 MB] || 13240_NICER_J0030_MassRadius_1080.mp4 (1920x1080) [301.1 MB] || 13240_NICER_J0030_MassRadius_Best_1080.mp4 (1920x1080) [804.5 MB] || 13240_NICER_J0030_MassRadius_SRT_Captions.en_US.srt [5.9 KB] || 13240_NICER_J0030_MassRadius_SRT_Captions.en_US.vtt [5.9 KB] || 13240_NICER_J0030_MassRadius_ProRes_1920x1080_2997.mov (1920x1080) [1.9 GB] || ", "hits": 169 }, { "id": 13429, "url": "https://svs.gsfc.nasa.gov/13429/", "result_type": "Produced Video", "release_date": "2019-12-10T10:00:00-05:00", "title": "OSIRIS-REx Sample Site Selection Trailer", "description": "Trailer for the sample site selection announcement for OSIRIS-REx, set to take place on December 12, 2019 at 1:00 PM EST/10:00 AM PST at AGU in San Francisco.Music is \"Oceana\" from Universal Production Music. || OREX_TRAILER_THUMB.jpg (3840x2160) [1.2 MB] || 13429_OSIRISREX_TRAILER_MASTER.01966_searchweb.png (320x180) [43.7 KB] || 13429_OSIRISREX_TRAILER_MASTER.01966_thm.png (80x40) [4.5 KB] || 13429_OSIRISREx_TRAILER_MASTER_facebook_720.mp4 (1280x720) [89.7 MB] || 13429_OSIRISREx_TRAILER_MASTER_twitter_720.mp4 (1280x720) [15.7 MB] || 13429_OSIRISREx_TRAILER_MASTER.webm (960x540) [35.5 MB] || 13429_OSIRISREx_TRAILER_MASTER.mov (3840x2160) [4.0 GB] || Trailer_VO_Output.en_US.srt [1.1 KB] || Trailer_VO_Output.en_US.vtt [1.2 KB] || ", "hits": 18 }, { "id": 13343, "url": "https://svs.gsfc.nasa.gov/13343/", "result_type": "Produced Video", "release_date": "2019-10-16T10:00:00-04:00", "title": "Soundbites: Hubble Observes 1st Confirmed Interstellar Comet", "description": "Quick link to canned interview with Dr, Jennifer WisemanQuick link to canned interview with Dr. Ken CarpenterClick here for full feature about Hubble's view of comet 2I/Borisov.You can download the new image here. || comet_banner.png (2136x666) [2.2 MB] || comet_banner_print.jpg (1024x319) [67.0 KB] || comet_banner_searchweb.png (320x180) [82.3 KB] || comet_banner_thm.png (80x40) [4.4 KB] || ", "hits": 81 }, { "id": 13341, "url": "https://svs.gsfc.nasa.gov/13341/", "result_type": "Produced Video", "release_date": "2019-10-16T09:55:00-04:00", "title": "Hubble's New Image Of Interstellar Object", "description": "NASA’s Hubble Space Telescope has given astronomers their best look yet at an interstellar visitor – Comet 2I/Borisov – whose speed and trajectory indicates it is from outside of our Solar System.This Hubble image, taken on October 12, is the sharpest ever view of the comet. Hubble reveals a central concentration of dust around the solid icy nucleus. For more information, visit https://nasa.gov/hubble.Music Credits: \"Solar Pilgrims\" by Francois Vey [ SACEM ] Universal Production Music || ", "hits": 101 }, { "id": 4758, "url": "https://svs.gsfc.nasa.gov/4758/", "result_type": "Visualization", "release_date": "2019-10-16T00:00:00-04:00", "title": "The Path of Comet 2I/Borisov", "description": "Follow 2I/Borisov from September 2018 to April 2020 as it flies through our solar system. || flyby.0396_print.jpg (1024x576) [117.5 KB] || flyby.0396_searchweb.png (320x180) [71.4 KB] || flyby.0396_thm.png (80x40) [4.3 KB] || flyby_1080p30.mp4 (1920x1080) [11.4 MB] || flyby_720p30.mp4 (1280x720) [6.0 MB] || flyby_720p30.webm (1280x720) [2.4 MB] || flyby_dates (1920x1080) [0 Item(s)] || flyby_360p30.mp4 (640x360) [2.1 MB] || flyby_1080p30.mp4.hwshow [179 bytes] || ", "hits": 144 }, { "id": 4760, "url": "https://svs.gsfc.nasa.gov/4760/", "result_type": "Visualization", "release_date": "2019-10-16T00:00:00-04:00", "title": "Grand Average Precipitation Climatology", "description": "Grand Average Precipitation Climatology || grand_average_climatology2_black_print.jpg (1024x576) [128.5 KB] || grand_average_climatology2_black_searchweb.png (320x180) [87.7 KB] || grand_average_climatology2_black_thm.png (80x40) [8.0 KB] || grand_average_climatology2_black.tif (3840x2160) [80.5 MB] || ", "hits": 44 }, { "id": 13331, "url": "https://svs.gsfc.nasa.gov/13331/", "result_type": "Produced Video", "release_date": "2019-09-30T14:00:00-04:00", "title": "International Observe the Moon Night Celebrates 10 Years of Lunar Engagement", "description": "A trailer for the 10th annual International Observe the Moon Night, which will be held on October 5th. Watch this video on the NASA Goddard YouTube channel. || poster-VX-306421-00-00-02-09.jpg (1920x1080) [241.2 KB] || INOMN_TRAILER.00045_print.jpg (1024x576) [93.4 KB] || INOMN_TRAILER.00045_searchweb.png (320x180) [76.0 KB] || FACEBOOK_720_INOMN_TRAILER_facebook_720.mp4 (1280x720) [50.7 MB] || INOMN_TRAILER.mp4 (1920x1080) [50.4 MB] || INOMN_TRAILER.webm (960x540) [18.0 MB] || TWITTER_720_INOMN_TRAILER_twitter_720.mp4 (1280x720) [8.3 MB] || 13331_Observe_the_Moon.en_US.srt [44 bytes] || 13331_Observe_the_Moon.en_US.vtt [57 bytes] || ", "hits": 126 }, { "id": 4720, "url": "https://svs.gsfc.nasa.gov/4720/", "result_type": "Visualization", "release_date": "2019-09-06T10:00:00-04:00", "title": "CGI Moon Kit", "description": "These color and elevation maps are designed for use in 3D rendering software. They are created from data assembled by the Lunar Reconnaissance Orbiter camera and laser altimeter instrument teams.", "hits": 43262 }, { "id": 31052, "url": "https://svs.gsfc.nasa.gov/31052/", "result_type": "Hyperwall Visual", "release_date": "2019-08-27T00:00:00-04:00", "title": "Revisiting Apollo Landing Sites", "description": "The six Apollo landing sites as imager by LROC || revisiting_apollo_landing_sites_LROC_print.jpg (1024x576) [174.3 KB] || revisiting_apollo_landing_sites_LROC.png (3840x2160) [6.2 MB] || revisiting_apollo_landing_sites_LROC_searchweb.png (320x180) [51.2 KB] || revisiting_apollo_landing_sites_LROC_thm.png (80x40) [3.6 KB] || revisiting_apollo_landing_sites_LROC.hwshow [121 bytes] || ", "hits": 30474 }, { "id": 40385, "url": "https://svs.gsfc.nasa.gov/gallery/arctic-campaigns-produced-videos/", "result_type": "Gallery", "release_date": "2019-08-23T00:00:00-04:00", "title": "Operation IceBridge Arctic Campaigns: Produced Videos ", "description": "No description available.", "hits": 17 }, { "id": 13264, "url": "https://svs.gsfc.nasa.gov/13264/", "result_type": "Produced Video", "release_date": "2019-08-01T14:00:00-04:00", "title": "Satellites Aid Active Fire Response", "description": "Complete transcript available. || Satellites_Aid_Active_Fire_Response_Final.00300_print.jpg (1024x576) [36.0 KB] || Satellites_Aid_Active_Fire_Response_Final.00300_searchweb.png (320x180) [52.7 KB] || Satellites_Aid_Active_Fire_Response_Final.00300_web.png (320x180) [52.7 KB] || Satellites_Aid_Active_Fire_Response_Final.00300_thm.png (80x40) [3.8 KB] || Satellites_aid_active_fire_response_Final.mov (1920x1280) [2.0 GB] || Satellites_Aid_Active_Fire_Response_Final.mp4 (1920x1080) [257.5 MB] || Satellites_aid_active_fire_response_Final.webm (1920x1280) [20.8 MB] || Satellites_Aid_Active_Fire_Response_Final.en_US.srt [3.4 KB] || Satellites_Aid_Active_Fire_Response_Final.en_US.vtt [3.4 KB] || ", "hits": 29 }, { "id": 4743, "url": "https://svs.gsfc.nasa.gov/4743/", "result_type": "Visualization", "release_date": "2019-07-30T00:00:00-04:00", "title": "Greenland's Jakobshavn Region: Three Simulated Greenland Ice Sheet Response Scenarios: 2008 - 2300", "description": "The Greenland Ice Sheet holds enough water to raise the world’s sea level by over 7 meters (23 feet). Rising atmosphere and ocean temperatures have led to an ice loss equivalent to over a centimeter increase in global mean sea-level between 1991 and 2015. Large outlet glaciers, rivers of ice moving to the sea, drain the ice from the interior of Greenland and cause the outer margins of the ice sheet to recede. Improvements in measuring the ice thickness in ice sheets is enabling better simulation of the flow in outlet glaciers, which is key to predicting the retreat of ice sheets into the future.Recently, a simulation of the effects of outlet glacier flow on ice sheet thickness coupled with improved data and comprehensive climate modeling for differing future climate scenarios has been used to estimate Greenland’s contribution to sea-level over the next millennium. Greenland could contribute 5–34 cm (2-13 inches) to sea-level by 2100 and 11–162 cm (4-64 inches) by 2200, with outlet glaciers contributing 19–40 % of the total mass loss. The analysis shows that uncertainties in projecting mass loss are dominated by uncertainties in climate scenarios and surface processes, followed by ice dynamics. Uncertainties in ocean conditions play a minor role, particularly in the long term. Greenland will very likely become ice-free within a millennium without significant reductions in greenhouse gas emissions.Three visualizations of the evolution of the Jakobshavn region of the Greenland Ice Sheet between 2008 and 2300 based on three different climate scenarios are shown below. Each scenario is described briefly in the caption under each visualization. Each of the three visualizations are provided with a date, colorbar and a distance scale as well as without. The regions shown in a violet color are exposed areas of the Greenland bed that were covered by the ice sheet in 2008.The data sets used for these animations are the control (“CTRL”) simulations and were produced with the open-source Parallel Ice Sheet Model . All data sets for this study are publicly available at the NSF Arctic Data Center || ", "hits": 23 }, { "id": 13200, "url": "https://svs.gsfc.nasa.gov/13200/", "result_type": "Produced Video", "release_date": "2019-07-29T10:00:00-04:00", "title": "NASA’s TESS Finds Three New Worlds", "description": "This infographic illustrates key features of the TOI 270 system, located about 73 light-years away in the southern constellation Pictor. The three known planets were discovered by NASA’s Transiting Exoplanet Survey Satellite through periodic dips in starlight caused by each orbiting world. Insets show information about the planets, including their relative sizes, and how they compare to Earth. Temperatures given for TOI 270’s planets are equilibrium temperatures, calculated without the warming effects of any possible atmospheres. Credit: NASA’s Goddard Space Flight Center/Scott Wiessinger || TOI_270_Infographic_Final_print.jpg (1024x576) [64.1 KB] || TOI_270_Infographic_Final.png (5760x3240) [17.4 MB] || TOI_270_Infographic_Final.jpg (5760x3240) [2.0 MB] || TOI_270_Infographic_Final-halfsize.png (2880x1620) [5.4 MB] || TOI_270_Infographic_Final-halfsize.jpg (2880x1620) [484.0 KB] || TOI_270_Infographic_Final_searchweb.png (320x180) [47.7 KB] || TOI_270_Infographic_Final_thm.png (80x40) [4.9 KB] || ", "hits": 210 }, { "id": 4706, "url": "https://svs.gsfc.nasa.gov/4706/", "result_type": "Visualization", "release_date": "2019-07-28T00:00:00-04:00", "title": "Greenland's Hiawatha Crater", "description": "This visualization shows the location of the Hiawatha Glacier near Inglefield Land in northwest Greenland. The surface of the ice sheet fades away to show the impact crater discovered beneath the ice sheet. A red cylinder shows the best-fit rim of the impact crater and a measuring stick shows that the diameter of the crater is more than 31 kilometers across. The size of the crater is compared to the cities of Washington, DC and Paris, France.The visualization also shows how the scientists from Germany's Alfred Wegener Institute (AWI) flew the Polar 6 aircraft (a DC-3T) to collect radar data over the Hiawatha impact crater. The radar data is shown in detail as curtains of the radar data are dissolved away to display the layers of the ice sheet in the interior of the crater. || Hiawatha.0590_print.jpg (1024x576) [150.4 KB] || Hiawatha.0590_searchweb.png (320x180) [88.4 KB] || Hiawatha.0590_thm.png (80x40) [6.2 KB] || 4706_Hiawatha_Crater.webmhd.webm (1080x606) [23.5 MB] || 4706_Hiawatha_Crater.mp4 (1920x1080) [228.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || 4706_Hiawatha_Crater.en_US.vtt [2.1 KB] || 4706_Hiawatha_Crater.en_US.srt [2.0 KB] || Hiawatha_Prores_4k.mp4 (3840x2160) [566.2 MB] || 4706_Hiawatha_Crater.mov (1920x1080) [1.9 GB] || Hiawatha_Prores_4k.mov (3840x2160) [7.6 GB] || ", "hits": 56 }, { "id": 4738, "url": "https://svs.gsfc.nasa.gov/4738/", "result_type": "Visualization", "release_date": "2019-07-24T00:00:00-04:00", "title": "Northeast Regional View of Three Simulated Greenland Ice Sheet Response Scenarios: 2008 - 2300", "description": "The Greenland Ice Sheet holds enough water to raise the world’s sea level by over 7 meters (23 feet). Rising atmosphere and ocean temperatures have led to an ice loss equivalent to over a centimeter increase in global mean sea-level between 1991 and 2015. Large outlet glaciers, rivers of ice moving to the sea, drain the ice from the interior of Greenland and cause the outer margins of the ice sheet to recede. Improvements in measuring the ice thickness in ice sheets is enabling better simulation of the flow in outlet glaciers, which is key to predicting the retreat of ice sheets into the future.Recently, a simulation of the effects of outlet glacier flow on ice sheet thickness coupled with improved data and comprehensive climate modeling for differing future climate scenarios has been used to estimate Greenland’s contribution to sea-level over the next millennium. Greenland could contribute 5–34 cm (2-13 inches) to sea-level by 2100 and 11–162 cm (4-64 inches) by 2200, with outlet glaciers contributing 19–40 % of the total mass loss. The analysis shows that uncertainties in projecting mass loss are dominated by uncertainties in climate scenarios and surface processes, followed by ice dynamics. Uncertainties in ocean conditions play a minor role, particularly in the long term. Greenland will very likely become ice-free within a millennium without significant reductions in greenhouse gas emissions.Three visualizations of the evolution of the northeastern region of the Greenland Ice Sheet between 2008 and 2300 based on three different climate scenarios are shown below. Each scenario is described briefly in the caption under each visualization. Each of the three visualizations are provided with a date, colorbar and a distance scale as well as without. The regions shown in a violet color are exposed areas of the Greenland bed that were covered by the ice sheet in 2008.The data sets used for these animations are the control (“CTRL”) simulations and were produced with the open-source Parallel Ice Sheet Model . All data sets for this study are publicly available at the NSF Arctic Data Center || ", "hits": 15 }, { "id": 4739, "url": "https://svs.gsfc.nasa.gov/4739/", "result_type": "Visualization", "release_date": "2019-07-24T00:00:00-04:00", "title": "Northwest Regional View of Three Simulated Greenland Ice Sheet Response Scenarios: 2008 - 2300", "description": "The Greenland Ice Sheet holds enough water to raise the world’s sea level by over 7 meters (23 feet). Rising atmosphere and ocean temperatures have led to an ice loss equivalent to over a centimeter increase in global mean sea-level between 1991 and 2015. Large outlet glaciers, rivers of ice moving to the sea, drain the ice from the interior of Greenland and cause the outer margins of the ice sheet to recede. Improvements in measuring the ice thickness in ice sheets is enabling better simulation of the flow in outlet glaciers, which is key to predicting the retreat of ice sheets into the future.Recently, a simulation of the effects of outlet glacier flow on ice sheet thickness coupled with improved data and comprehensive climate modeling for differing future climate scenarios has been used to estimate Greenland’s contribution to sea-level over the next millennium. Greenland could contribute 5–34 cm (2-13 inches) to sea-level by 2100 and 11–162 cm (4-64 inches) by 2200, with outlet glaciers contributing 19–40 % of the total mass loss. The analysis shows that uncertainties in projecting mass loss are dominated by uncertainties in climate scenarios and surface processes, followed by ice dynamics. Uncertainties in ocean conditions play a minor role, particularly in the long term. Greenland will very likely become ice-free within a millennium without significant reductions in greenhouse gas emissions.Three visualizations of the evolution of the northwest region of the Greenland Ice Sheet between 2008 and 2300 based on three different climate scenarios are shown below. Each scenario is described briefly in the caption under each visualization. Each of the three visualizations are provided with a date, colorbar and a distance scale as well as without. The regions shown in a violet color are exposed areas of the Greenland bed that were covered by the ice sheet in 2008.The data sets used for these animations are the control (“CTRL”) simulations and were produced with the open-source Parallel Ice Sheet Model . All data sets for this study are publicly available at the NSF Arctic Data Center || ", "hits": 13 }, { "id": 13223, "url": "https://svs.gsfc.nasa.gov/13223/", "result_type": "Produced Video", "release_date": "2019-06-27T09:00:00-04:00", "title": "TESS Discovers Its Tiniest World To Date", "description": "NASA’s Transiting Exoplanet Survey Satellite has confirmed the tiniest planet in its catalog so far — one of three discovered around a bright, nearby star called L 98-59. As shown in the illustrations in this video, all could occupy the “Venus zone,” the range of distances from the star where a Venus-like atmosphere is possible. The outermost planet also has the potential for a Neptune-like atmosphere. Credit: NASA’s Goddard Space Flight CenterMusic: \"Autumn Rush\" from Killer TracksComplete transcript available.Watch this video on the NASA Goddard YouTube channel. || tess_smallest_planet_preview.jpg (1920x1080) [288.5 KB] || tess_smallest_planet_preview_print.jpg (1024x576) [118.1 KB] || tess_smallest_planet_preview_searchweb.png (320x180) [53.2 KB] || tess_smallest_planet_preview_web.png (320x180) [53.2 KB] || tess_smallest_planet_preview_thm.png (80x40) [5.5 KB] || tess_smallest_planet_HQ.mp4 (1920x1080) [245.9 MB] || tess_smallest_planet_LQ.mp4 (1920x1080) [190.0 MB] || tess_smallest_planet_prores.mov (1920x1080) [1.3 GB] || tess_smallest_planet_HQ.webm (1920x1080) [14.8 MB] || tess_smallest_planet.en_US.srt [1.9 KB] || tess_smallest_planet.en_US.vtt [1.9 KB] || ", "hits": 124 }, { "id": 4721, "url": "https://svs.gsfc.nasa.gov/4721/", "result_type": "Visualization", "release_date": "2019-06-19T14:00:00-04:00", "title": "Three Simulated Greenland Ice Sheet Response Scenarios: 2008 - 2300", "description": "The Greenland Ice Sheet holds enough water to raise the world’s sea level by over 7 meters (23 feet). Rising atmosphere and ocean temperatures have led to an ice loss equivalent to over a centimeter increase in global mean sea-level between 1991 and 2015. Large outlet glaciers, rivers of ice moving to the sea, drain the ice from the interior of Greenland and cause the outer margins of the ice sheet to recede. Improvements in measuring the ice thickness in ice sheets is enabling better simulation of the flow in outlet glaciers, which is key to predicting the retreat of ice sheets into the future.Recently, a simulation of the effects of outlet glacier flow on ice sheet thickness coupled with improved data and comprehensive climate modeling for differing future climate scenarios has been used to estimate Greenland’s contribution to sea-level over the next millennium. Greenland could contribute 5–34 cm (2-13 inches) to sea-level by 2100 and 11–162 cm (4-64 inches) by 2200, with outlet glaciers contributing 19–40 % of the total mass loss. The analysis shows that uncertainties in projecting mass loss are dominated by uncertainties in climate scenarios and surface processes, followed by ice dynamics. Uncertainties in ocean conditions play a minor role, particularly in the long term. Greenland will very likely become ice-free within a millennium without significant reductions in greenhouse gas emissions.Three visualizations of the evolution of the Jakobshavn region of the Greenland Ice Sheet between 2008 and 2300 based on three different climate scenarios are shown below. The camera zooms in slowly as the ice sheet retreats and pulls out to a view of the entire ice sheet in the year 2300. Each scenario is described briefly in the caption under each visualization. Each of the three visualizations are provided with a date, colorbar and a distance scale as well as without. The regions shown in a violet color are exposed areas of the Greenland bed that were covered by the ice sheet in 2008.The data sets used for these animations are the control (“CTRL”) simulations and were produced with the open-source Parallel Ice Sheet Model (www.pism-docs.org). All data sets for this study are publicly available at https://arcticdata.io (doi:10.18739/A2Z60C21V). || ", "hits": 58 }, { "id": 4722, "url": "https://svs.gsfc.nasa.gov/4722/", "result_type": "Visualization", "release_date": "2019-06-19T14:00:00-04:00", "title": "Jakobshavn Regional View of Three Simulated Greenland Ice Sheet Response Scenarios: 2008 - 2300", "description": "The Greenland Ice Sheet holds enough water to raise the world’s sea level by over 7 meters (23 feet). Rising atmosphere and ocean temperatures have led to an ice loss equivalent to over a centimeter increase in global mean sea-level between 1991 and 2015. Large outlet glaciers, rivers of ice moving to the sea, drain the ice from the interior of Greenland and cause the outer margins of the ice sheet to recede. Improvements in measuring the ice thickness in ice sheets is enabling better simulation of the flow in outlet glaciers, which is key to predicting the retreat of ice sheets into the future.Recently, a simulation of the effects of outlet glacier flow on ice sheet thickness coupled with improved data and comprehensive climate modeling for differing future climate scenarios has been used to estimate Greenland’s contribution to sea-level over the next millennium. Greenland could contribute 5–34 cm (2-13 inches) to sea-level by 2100 and 11–162 cm (4-64 inches) by 2200, with outlet glaciers contributing 19–40 % of the total mass loss. The analysis shows that uncertainties in projecting mass loss are dominated by uncertainties in climate scenarios and surface processes, followed by ice dynamics. Uncertainties in ocean conditions play a minor role, particularly in the long term. Greenland will very likely become ice-free within a millennium without significant reductions in greenhouse gas emissions.Three visualizations of the evolution of the Jakobshavn region of the Greenland Ice Sheet between 2008 and 2300 based on three different climate scenarios are shown below. Each scenario is described briefly in the caption under each visualization. Each of the three visualizations are provided with a date, colorbar and a distance scale as well as without. The regions shown in a violet color are exposed areas of the Greenland bed that were covered by the ice sheet in 2008.The data sets used for these animations are the control (“CTRL”) simulations and were produced with the open-source Parallel Ice Sheet Model (www.pism-docs.org). All data sets for this study are publicly available at https://arcticdata.io (doi:10.18739/A2Z60C21V). || ", "hits": 33 }, { "id": 4727, "url": "https://svs.gsfc.nasa.gov/4727/", "result_type": "Visualization", "release_date": "2019-06-19T14:00:00-04:00", "title": "Greenland View of Three Simulated Greenland Ice Sheet Response Scenarios: 2008 - 2300", "description": "The Greenland Ice Sheet holds enough water to raise the world’s sea level by over 7 meters (23 feet). Rising atmosphere and ocean temperatures have led to an ice loss equivalent to over a centimeter increase in global mean sea-level between 1991 and 2015. Large outlet glaciers, rivers of ice moving to the sea, drain the ice from the interior of Greenland and cause the outer margins of the ice sheet to recede. Improvements in measuring the ice thickness in ice sheets is enabling better simulation of the flow in outlet glaciers, which is key to predicting the retreat of ice sheets into the future.Recently, a simulation of the effects of outlet glacier flow on ice sheet thickness coupled with improved data and comprehensive climate modeling for differing future climate scenarios has been used to estimate Greenland’s contribution to sea-level over the next millennium. Greenland could contribute 5–34 cm (2-13 inches) to sea-level by 2100 and 11–162 cm (4-64 inches) by 2200, with outlet glaciers contributing 19–40 % of the total mass loss. The analysis shows that uncertainties in projecting mass loss are dominated by uncertainties in climate scenarios and surface processes, followed by ice dynamics. Uncertainties in ocean conditions play a minor role, particularly in the long term. Greenland will very likely become ice-free within a millennium without significant reductions in greenhouse gas emissions.Three visualizations of the evolution of the Greenland Ice Sheet between 2008 and 2300 based on three different climate scenarios are shown below. Each scenario is described briefly in the caption under each visualization. Each of the three visualizations are provided with a date and colorbar as well as without. The regions shown in a violet color are exposed areas of the Greenland bed that were covered by the ice sheet in 2008.The data sets used for these animations are the control (“CTRL”) simulations and were produced with the open-source Parallel Ice Sheet Model (www.pism-docs.org). All data sets for this study are publicly available at https://arcticdata.io (doi:10.18739/A2Z60C21V). || ", "hits": 127 }, { "id": 13221, "url": "https://svs.gsfc.nasa.gov/13221/", "result_type": "Produced Video", "release_date": "2019-06-10T10:00:00-04:00", "title": "NASA Tech on SpaceX Falcon Heavy Launch - Media Telecon Resources", "description": "NASA is sending four technology missions that will help improve future spacecraft design and performance into space on the next SpaceX Falcon Heavy rocket launch. Experts will discuss these technologies, and how they complement NASA’s Moon to Mars exploration plans, during a media teleconference Monday, June 10 at 1 p.m. EDT.Audio of the teleconference will be streamed live online at: https://www.nasa.gov/liveParticipants in the briefing will be:Jim Reuter, acting associate administrator of NASA’s Space Technology Mission Directorate, will discuss how technology drives exploration to the Moon and beyond.Jill Seubert, deputy principal investigator for the Deep Space Atomic Clock at NASA’s Jet Propulsion Laboratory, will discuss how to advance exploration in deep space with a miniaturized, ultra-precise, mercury-ion atomic clock that is orders of magnitude more stable than today’s best navigation clocks.Don Cornwell, director of the Advanced Communications and Navigation Division of NASA’s Space Communications and Navigation program, will discuss how a more stable, space-based atomic clock could benefit future missions to the Moon and Mars.Christopher McLean, principal investigator for NASA’s Green Propellant Infusion Mission (GPIM) at Ball Aerospace, will discuss the demonstration of a green alternative to conventional chemical propulsion systems for next-generation launch vehicles and spacecraft. Joe Cassady, executive director for space at Aerojet Rocketdyne, will discuss the five thrusters and propulsion system aboard GPIM.Nicola Fox, director of the Heliophysics Division of NASA’s Science Mission Directorate, will discuss Space Environment Testbeds and the importance of protecting satellites from space radiation.Richard Doe, payload program manager for the Enhanced Tandem Beacon Experiment at SRI International, will discuss how a pair of NASA CubeSats will work with six satellites of the National Oceanographic and Atmospheric Administration’s (NOAA’s) COSMIC-2 mission to study disruptions of signals that pass through Earth’s upper atmosphere.To participate in the teleconference, media must contact Clare Skelly at 202-358-4273 or clare.a.skelly@nasa.gov by 10 a.m. June 10. Media questions may be submitted on Twitter during the teleconference using the hashtag #askNASA.NASA’s four missions will share a ride on the Falcon Heavy with about 20 satellites from government and research institutions that make up the Department of Defense’s Space Test Program-2 (STP-2) mission. SpaceX and the U.S. Air Force Space and Missile Systems Center, which manages STP-2, are targeting 11:30 p.m. Saturday, June 22, for launch from historic Launch Complex 39A at NASA’s Kennedy Space Center in Florida.Charged with returning astronauts to the Moon within five years, NASA’s Artemis lunar exploration plans are based on a two-phase approach: the first is focused on speed – landing astronauts on the Moon by 2024 – while the second will establish a sustained human presence on and around the Moon by 2028. We will use what we learn on the Moon to prepare to send astronauts to Mars. The technology missions on this launch will advance a variety of future exploration missions.For more information about NASA’s Moon to Mars exploration plans, visit:https://www.nasa.gov/moontomarsFor more information about the NASA technologies aboard this launch, visit:https://www.nasa.gov/spacexLearn more about NASA’s Deep Space Atomic Clock: https://www.nasa.gov/mission_pages/tdm/clock/index.htmlLearn more about NASA’s Green Propellant Infusion Mission: https://www.nasa.gov/mission_pages/tdm/green/index.htmlSPACE TEST PROGRAM-2 || ", "hits": 42 }, { "id": 30805, "url": "https://svs.gsfc.nasa.gov/30805/", "result_type": "Hyperwall Visual", "release_date": "2019-06-10T10:00:00-04:00", "title": "Hubble: Galaxies Across Space and Time", "description": "This film explores galaxies within a Hubble observation looking deep into space and across ten billion years of cosmic history. || hgast-sample_frame-1920x1080.png (1920x1080) [2.2 MB] || hgast-sample_frame-1920x1080_print.jpg (1024x576) [27.0 KB] || hgast-sample_frame-1920x1080_searchweb.png (320x180) [57.0 KB] || hgast-sample_frame-1920x1080_thm.png (80x40) [3.3 KB] || hgast-1920x1080.webm (1920x1080) [100.7 MB] || hgast-1920x1080.m4v (1920x1080) [138.5 MB] || hgast-3840x2160p30.mp4 (3840x2160) [581.6 MB] || ", "hits": 159 } ] }